23rd Australian INSTITUTE of Physics Congress · 2. The registration desk will be open for the duration of the congress and will be your main point of contact for all congress related

Image credit: LIGO/R. Hurt (Caltech-IPAC)

9-13 December 2018Perth, Western Australia

Congress Handbook

23rd Australian INSTITUTE of Physics CongressJOINT WITHAUSTRALIAN OPTICAL SOCIETY (AOS) CONFERENCE;43RD AUSTRALIAN CONFERENCE ON OPTICAL FIBRE TECHNOLOGY (ACOFT);2018 CONFERENCE ON OPTOELECTRONIC AND MICROELECTRONIC MATERIALS AND DEVICES (COMMAD 2018)

23rd Australian Institute of Physics Congress 2018 – HANDBOOK2

23rd Australian INSTITUTE of Physics Congress

9-13 December 2018Perth, Western Australia

Table of contents

AIP Congress Committee Welcome ........................................................................................................................................... 3

AIP President’s Welcome ................................................................................................................................................................. 4

AOS President’s Welcome................................................................................................................................................................ 5

University of Western Australia Physics Head’s Welcome ............................................................................................. 6

COMMAD Chair Welcome ................................................................................................................................................................ 6

Acknowledgements ............................................................................................................................................................................ 7

AIP Congress Code of Conduct .................................................................................................................................................... 8

Useful Information ............................................................................................................................................................................... 9

Congress App .......................................................................................................................................................................................12

Social Functions ..................................................................................................................................................................................12

Workshops .............................................................................................................................................................................................13

Plenary and Keynote speakers ....................................................................................................................................................15

Program ...................................................................................................................................................................................................28

Venue maps ..........................................................................................................................................................................................42

Sponsors and Exhibitors .................................................................................................................................................................45

Exhibition Floorplan ...........................................................................................................................................................................52

Poster Program ...................................................................................................................................................................................53

Presenting Authors ............................................................................................................................................................................58

23rd Australian Institute of Physics Congress 2018 – HANDBOOK 3

AIP Congress Committee Welcome

This week’s proceedings comprise the 23rd Australian Institute of Physics Biennial Congress, the Australian Optical Society (AOS) Conference, the 43rd Australian Conference on Optical Fibre Technology (ACOFT), the Conference on Optoelectronic and Microelectronic Materials and Devices (COMMAD 2018). On behalf of all of these, welcome to Perth!

The scientific program reflects the breadth of physical sciences and technology in Australia, with topics ranging from the very fundamental to the very applied. The program also reflects the value placed on all facets of the physics-related activities – encompassing academic research, teaching and education, and industrial and technological applications.

In planning this year’s congress, the program and organising committees have had a particular view towards diversity and inclusivity. We are pleased that the program achieves a good gender balance amongst the keynote and plenary speakers, and we reaffirm our commitment to the principles of diversity, gender balance and inclusivity. This commitment clearly reflects current priorities amongst our registered participants: the ‘Diversity and Equity Group in Australian Physics’ session was booked out in next to no time! Our apologies to those who missed out.

Please take kind note of our sponsors and exhibitors, listed on page 45. This week’s special sessions, plenary presentations and networking events – free to all participants – have been made possible by their generous support which we gratefully acknowledge.

Physics, and science in general, have a lot to offer to the society we live in. Few doubt the evident contributions of our discipline to scientific advances and its relevance to our technology-based industries – and we are here to celebrate these. Yet, surely, the discerning and quantitative way of thinking on which we pride ourselves is a crucial element not just of a more productive society, but more broadly of a smarter society. “To think like a physicist” should be a badge of honour that is worn with pride, not just within the confines of the research lab or lecture theatre but in the arena of public debate, where our society’s future direction is at stake. Alongside the in-depth scientific programme, we hope to see elements of this broader discussion about the role of our discipline in society in the lecture theatres or during the social events!

On behalf of all members of the organising and program committee, I would like to wish you an enjoyable time at the congress, and hope you take away some new and profound scientific insights during your time here in Western Australia.

Gerd Schröder-TurkAIP Congress Organising Committee Chair


AIP President’s Welcome

Welcome to the 23rd Australian Institute of Physics Congress, held jointly with the Australian Optical Society Conference, the 43rd Australian Conference on Optics and Fibre Technology and the 2018 Conference on Optoelectronic and Microelectronic Materials and Devices.

The Congress provides one of the best local opportunities for physicists from a wide range of research, education, government and industry to share ideas, network and hear talks from our distinguished plenary and keynote speakers as well as from other colleagues presenting in the broader program.

It is great to see Congress held in Perth – the first time this millennium! And it is great to see the strength of the program, which between the astronomy and gravitational wave streams and the joint optics conferences is very well aligned with recent Nobel prizes. Both these geographic and topical alignments are surely signs of the strength and interest in the physics community in Australia.

That strength is matched by the efforts of all those involved in organising this Congress.

On behalf of the Australian Institute of Physics, thank you to all those involved, particularly to the local organising committee. We hope all delegates enjoy an informative and rewarding Congress.

Andrew Peele and Jodie BradbyPresident and Vice-President, Australian Institute of Physics


AOS President’s Welcome

I would like to start by welcoming you all to the ACOFT / AOS Conference stream of this Congress.

The AOS is delighted to partner again with AIP in this congress to hold our annual conference. We hope that the Australian and New Zealand optics and photonics community will benefit from this excellent opportunity, not only to renew contacts within our community, but to engage with the wider physics community.

Our conferences in this Congress are the 43rd Australian Conference on Optical Fibre Technology (ACOFT) and the AOS Conference, held biennially with the AIP Congress for many years now. AOS also runs ANZCOP and ACOLS, and we are actively reviewing ways to streamline these conferences to provide the best support for the Australasian optics community. Supporting conferences is a major activity of AOS, and I encourage you to get involved in AOS to help steer future events.

I congratulate the organizers on bringing together such a strong program. The invited speakers are especially exciting, covering some of the hottest topics in optics and photonics. It is particularly pleasing to see good diversity in this group.

It’s great to be in Perth again, only the third time we have held a conference here (ANZCOP 2013 and ACOFT 1985).

I would like to thank everyone who has contributed to making this event a success: the organising committee and the members of the TPC whose expertise and time is so important. I particularly want to thank Robert McLaughlin who has so ably chaired the TPC for the AOS/ACOFT stream and coordinated so many aspects of our involvement in this Congress.

Enjoy the event and Perth, be inspired by the great speakers, renew old friendships and make new ones. Make the most of this annual congregation of Australasian optics and photonics researchers, and physicists.

Simon FlemingAOS President


University of Western Australia Physics Head’s Welcome

We are very pleased to be hosting the 23rd Australian Institute of Physics Congress and the Australian Optical Society Conference (AOS), the 43rd Australian Conference on Optical Fibre Technology (ACOFT), and the 2018 Conference on Optoelectronic and Microelectronic Materials and Devices (COMMAD) in our leafy campus, overlooking the picturesque Matilda Bay. The conference venue is conveniently situated about 8 minutes from Perth CBD, 10 minutes from the stunning Cottesloe beach, with nearby Kings Park and Botanic Garden, leisure and dining. We take great pride in welcoming you all to the University of Western Australia.

The biennial AIP Congress, the AOS, ACOFT and COMMAD Conferences, are the premier national forums to present and discuss progress in physics related research in both fundamental and applied areas. This is an exciting time for physics and this grand event brings together leading researchers in almost all fields of physics. We are delighted to have such an eminent list of speakers from many different countries. This will be a great opportunity to network, to exchange inspiring new ideas, to strengthen existing collaborations and to forge new partnerships.

We look forward to seeing you in Perth, and hope you will find the conferences informative and valuable.

Jingbo WangHead of Physics Department, University of Western Australia

COMMAD CHAIR Welcome

Welcome to the 2018 Conference on Optoelectronic and Microelectronic Materials and Devices, held jointly with the 23rd Australian Institute of Physics Congress, the Australian Optical Society Conference, and the 43rd Australian Conference on Optics and Fibre Technology. COMMAD is delighted to partner for the first time with AIP and AOS. It is great to welcome you at this joint conference event in the beautiful Perth on the Indian Ocean coast of Australia.

COMMAD would like to thank the Australian Nanotechnology Network for supporting the attendance of students and early career researchers and The University of Western Australia for hosting the meeting. In addition, we are very delighted to be able to partner with the Australian National Fabrication Facility and offer a Short Course on Nanofabrication Technologies with a motto of Engineering your Imagination.

Please enjoy the event, the beautiful campus of UWA, Perth and Western Australia.

Mariusz MartyniukCOMMAD


Acknowledgements

CONGRESS ORGANISING COMMITTEEGerd Schroeder-Turk, ChairIgor Bray, Co-chairIan McArthur, Co-chairAlmantas Pivrikas, SecretaryRon Burman, TreasurerDavid BlairJodie BradbySharon EyerKetesse HansenMariusz MartyniukRobert McLaughlinStuart MidgleyHalina Rubinsztein-DunlopAna-Suncana SmithGeoff SwanCathryn TrottKathryn Wilson

AIP EXECUTIVEAndrew Peele, PresidentJodie Bradby, Vice PresidentKirrily Rule, Honorary SecretaryJudith Pollard, Honorary TreasurerStephen Collins, Honorary RegistrarWarrick Couch, Immediate Past PresidentOlivia Samardzic, Special Project Office

PROGRAM COMMITTEEMichael Tobar, ChairJingbo Wang, Co-chairBruce Gardiner, Secretary Igor BrayBrett Carter Evenlyne DeplazesSimon DoeMartin Ebert Ben EggletonLorenzo FaraoneSimon FlemingMatthew HoleMikhail KostylevPegah Fatemah MaasoumiMariusz MartyniukIan McArthurRobert McLaughlinAndrea MorelloMaria ParrappillyGerd Schroeder-TurkLister Staveley-SmithChris ValeAnton Wallner

CONGRESS SECRETARIAT

PO Box 6150, Kingston, ACT, 2604P: 02 6281 6624E: [email protected]: www.conferencelogistics.com.au

For assistance during the Congress, please phone the registration desk on 0498 435 169.

8

Acknowledgment of Country The Australian Institute of Physics Congress 2018 Committee acknowledges that the Congress is being held on Noongar land, and that Noongar people remain the spiritual and cultural custodians of their land, and continue to practise their values, languages, beliefs and knowledge.

AIP Congress Code of ConductOur congress is dedicated to providing a harassment-free experience for everyone, regardless of gender, gender identity and expression, age, sexual orientation, disability, physical appearance, body size, race, ethnicity, religion (or lack thereof), or technology choices. We do not tolerate harassment of congress participants in any form. Sexual language and imagery is not appropriate for any Congress venue, including talks, workshops, parties, Twitter and other online media. Congress participants violating these rules may be sanctioned or expelled from the congress without a refund at the discretion of the congress organisers.


Venue and registration

Congress venueUniversity of Western AustraliaCrawley CampusStirling Highway, Perth WA

RegistrationThe registration desk is located at the rear entrance of the University Club of Western Australia, in front of Seminar Rooms 1 and 2. The registration desk will be open for the duration of the congress and will be your main point of contact for all congress related enquiries.

You can contact the congress organisers on 0498 435 169 for the duration of the congress 9-13 December.

The registration desk will be open at the following times:

Sunday 9 December: 8.30am to 6.30pm Monday 10 December: 7.00am to 6.30pmTuesday 11 December: 7.30am to 6.00pm Wednesday 12 December: 7.30am to 7.30pmThursday 13 December: 7.30am to 6.00pm

Name badges Your official Congress name badge must be worn at all times as it is your entry to all congress sessions, the Exhibition Hall and social functions. Entry may be refused to anyone not wearing their name badge.

Catering and special requirementsAll catering served will be an informal stand-up buffet. Please note the locations for catering during the congress below as there will be a change on the last day:

Monday 10 December – Wednesday 12 December: Morning, afternoon teas and lunches will be served in the Banquet Hall at the University Club.

Thursday 13 December: Morning, afternoon teas and lunch will be served on the outdoor Terrace at the University Club.

Dietary requirements noted on your registration have been passed onto the catering staff for all congress related activities, including the main congress, workshops and social events.

Delegates who requested specific dietary requirements will have a special diet card included in the back of their name badge holder, and a separate table to pick up food. Please ask the catering staff to assist if required.

NOTE: Dietary requests will be catered for to the best of the venue’s ability. Individuals with severe allergies are requested to advise Conference Logistics prior to the congress of their requirements, and bring any allergy medication (EpiPen, Phenergan, etc.) as prescribed by your doctor to the congress and any associated function. Whilst due care is taken by the organisers and venue, individuals must take primary responsibility for their own health.

Internet access

Delegates should access their Eduroam accounts for Wi-Fi during the Congress. For any delegates who do not have Eduroam accounts there will be a limited number of Unifi guest network (UWA Wi-Fi network) passes available at the registration desk

Please note the Unifi network will be undergoing maintenance on Sunday 9 December and disruptions to the Wi-Fi network are expected. The rest of the week should not be affected.

useful information


Special requirements Every effort has been made to ensure people with special needs are catered for. If you have not previously advised the secretariat of any special dietary requirement or accessibility requirements, please see the staff at the registration desk as soon as possible.

Functions, workshops and exhibition

Congress functions

All programmed congress functions are ticketed events and require registration to attend. Please see the staff at the registration desk if you wish to purchase additional tickets. Your function tickets (except for the Welcome Reception) can be found in your name badge holder.

Workshops

Various workshops will run over the course of the congress and require registration to attend. All functions are now full. Please refer to the workshop ticket in your name badge holder for workshop details.

Exhibition hours

The exhibition will be held in the Banquet Hall at the University Club during the following days:

Monday 10 December: 7.30am to 6.30pmTuesday 11 December: 7.30am to 5.30pm Wednesday 12 December: 7.30am to 3.30pm

Sundowner poster session

Posters are located in the Banquet Hall, Lower Colonnade and the Banquet Hall foyer and will be available for viewing from Monday - Wednesday. An official Sundowner Poster Session will be run on Monday 10 December with drinks and snacks. During the poster session on Monday we invite delegates to vote on their favourite poster, after which a People’s Choice Poster Competition, sponsored by IEEE, will be awarded.

Poster presenters will be available near their posters during this Sundowner Poster Session. Please refer to the poster program on page 53 for more information on presenting posters.

Poster Session

Date: Monday 10 DecemberTime: 5.30pm – 6.30pmLocation: Banquet Hall

Sponsored by

General

Delegate list

A delegate list with name, organisation and state is available to be viewed on the congress app. Delegates who opted out of being included on the delegate list will not appear.

Dress code

The dress for all congress sessions and social functions is smart casual.


Lost and found

Please report any lost or found property to the registration desk.

Cloak room

There will be a cloak room available throughout the congress at the registration desk. Please note in regards to luggage there will be a limited amount of storage available so please confirm luggage store options with your hotel upon check in.

Mobile phones

As a courtesy to other delegates and speakers, please ensure all mobile phones are turned off or in ‘silent’ mode during all sessions and social functions.

Parking

There is a limited amount of paid parking available at the University of Western Australia. Delegates are recommended to park in long term parking spots along Hackett Drive and parking spots in and around the University Club P3. Please ensure you read all signage for fees and the maximum duration you can park.

For full details on venue parking please visit www.transport.uwa.edu.au/car-pooling/visitor

A car parking map can be found here: www.web.uwa.edu.au/__data/assets/pdf_file/0007/148948/UWA-PARKING-MAP_2017.pdf

Social media

Join the conversation by using the in-app social media page and adding the #AIPCongress2018 to your tweets, Facebook or Instagram posts.

Recording and photography

Unauthorised audio taping, video recording, digital taping or any other form of recording is strictly prohibited in congress sessions. Speakers who do not wish to have photographs taken of their slides must state this at the start of their presentation. The plenary sessions may be filmed or photographed for future educational opportunities by the Australian Institute of Physics.

By attending the congress, you agree to be photographed and/or filmed and give permission to the Australian institute of Physics and their affiliates, to use your likeness in commercial promotional and/or marketing materials. This permission is granted without expectation of compensation or other remuneration, now or into the future. Please contact Conference Logistics if you require further information.

Evaluation survey

An online evaluation survey will be available through the congress app at the end of the congress. It will also be emailed to all delegates following the congress. Delegates are encouraged to complete the congress evaluation as it assists in planning for future congresses.

Travel

AirlinesQantas 13 13 13 Virgin 13 67 89

TaxisBlack and White Cabs 13 32 22Swan Taxis 13 13 30

UberDownload the Uber app or visit the Uber website at www.uber.com


Congress AppThe AIP2018 app offers you a range of great ways to maximise your Congress experience, including:

• Creating your own program for ease of reference

• Viewing all the presenter’s abstracts and biographies

• Taking part in the in-congress social media stream

• Direct messaging other attendees, exhibitors and the event organisers

• Receiving alerts of any changes

• And much more!

To download the app follow these steps:

1. Go to your device’s store and search for the Conlog app.

2. Download the Conlog app to your device (free to download).

3. Log in using the appcode (AIP2018) and your unique pin you received via email

If you have misplaced your unique pin, please see the friendly staff at the registration desk for assistance.

Social FunctionsWelcome Reception

Date: Sunday 9 DecemberTime: 6.00pm – 8.00pmVenue: Ground Floor Terrace, the University Club,

University Western Australia

One ticket included with full registrations. Additional tickets available from the registration desk at $45 inc GST.

Sponsored by

Sundowner Poster Session

Date: Monday 10 December Time: 5.30pm – 6.30pmVenue: Terrace, The University Club, University

Western Australia

All delegates welcome, refer to the Sundowner Poster Session program on page 53 . A People’s

Choice Poster Competition, sponsored by IEEE, will be run during the Sundowner Poster Session. Delegates are invited to vote via the Congress App for their favourite poster.

Sponsored by

Congress Dinner

Date: Wednesday 12 December Time: 7.30pm – 10.00pmVenue: Ground Floor Terrace, the University Club,


The Congress Dinner will be a stand up, casual event within the grounds of the University of Western Australia. The dinner includes the presentation by Dame Julia Higgins.

One ticket included with full registrations. Additional tickets available from the registration desk at $75 inc GST.


Engineering your Imagination: ANFF Short Course on Nanofabrication Technologies

Date: Sunday 9 December Time: 10.00am – 4.30pmVenue: Auditorium, the University Club,


Delegates must register for this workshop, limited tickets available.

Diversity and Equity Group in Australian Physics (DE-GAP) Workshop (including brunch)

Date: Tuesday 11 December 2018Time: 10.00am - 1.00pmVenue: Seminar Room One, the University Club

Workshop FULL. Only registered delegates can attend. If you are on the waitlist, please see registration desk.

Sponsored by

Discussion: Theoretical and Mathematical Physics in Australia

Date: Tuesday 11 DecemberTime: 12.45pm – 1.15pmVenue: Arts Building, Room 10 [1.62]

Open to all delegates, spaces limited.

Physics in Education Group (PEG) Workshop (including High Tea)

Date: Tuesday 11 DecemberTime: 3.30pm - 4.30pmVenue: Club Restaurant, the University ClubTickets: $38 per person, limited tickets available

Sponsored by

The Secrets of Scientific Publishing

Workshop OneDate: Tuesday 11 DecemberTime: 1.30pm – 3.00pmVenue: Arts Building, Room 6 [G.62]

Workshop TwoDate: Wednesday 12 DecemberTime: 1.30pm – 3.00pmVenue: Arts Building, Room 6 [G.62]

Workshop FULL. Only registered delegates can attend. If you are on the waitlist, please see registration desk.

Teaching Nexus: Evolving Physics Education in our schools, Workshop One

Date: Wednesday 12 DecemberTime: 9.00am – 10.30amVenue: Physics Lab, University of Western

AustraliaFacilitator: Jason Dicker

Open to all delegates, spaces limited.

workshops


Teaching Nexus: Evolving Physics Education in our schools, Workshop Two

Date: Wednesday 12 DecemberTime: 11.30am - 12.30pmVenue: Computer Lab, University of

Western AustraliaFacilitator: Dr David Hoxley

Open to all delegates, spaces limited

Teaching Nexus: Evolving Physics Education in our School - PEG Workshop 3

Date: Wednesday 12 DecemberTime: 3.30pm – 5.00pmVenue: Physics Building, 215 Lecture

TheatreFacilitator: Professor David Blair


Decadal Plan Town Hall Meeting

Date: Thursday 13 DecemberTime: 12.45pm – 1.15pmVenue: Arts Building, Room 6 [G.62]


External events of interest – Public Lecture

In addition to the AIP 2018 program, the Australian Institute of Physics together with the Institute of Advanced Studies are co-sponsoring a Public Lecture on the grounds of the University of Western Australia. The Public Lecture will feature Marcus Aspelmeyer and Professor Rainer Weiss.

IMPORTANT NOTE: Attendance at the Public Lecture is not included in AIP Congress registration. You must confirm your free registration with the Institute of Advanced Studies.

Date: Tuesday 11 December Time: 5.45pm – 6.15pm: Presentation

by Markus Aspelmeyer, What is a Phonton?

6.30pm – 7.30pm: Lecture by Professor Rainer Weiss, Gravitational Waves

Venue: Octagon Theatre, University Western Australia

Tickets: Free, must register at www.ias.uwa.edu.au/lectures/physics

Co-sponsored by the Australian Institute of Physics and the Institute of Advanced Studies

Institute of Advanced Studies


plenary and keynote speakers

Professor Julia Yeomans

University of Oxford, UK

Julia Yeomans obtained her DPhil in Physics from the University of Oxford. She spent two years as a post-doc at Cornell University, then returned to the UK to become a Lecturer

at the University of Southampton. Soon after that, she joined the Rudolf Peierls Centre for Theoretical Physics at Oxford. She is currently Professor of Physics at Oxford and was instrumental in founding the Oxford Centre for Soft and Biological Matter. Julia works in theoretical and computational physics, particularly statistical physics, hydrodynamics, soft condensed matter and biological physics. Among her current research interests are active systems, complex fluids and the interactions of fluids with structured surfaces. She has been awarded the EPJE-Pierre Gilles de Gennes lecture prize and was elected a Fellow of the Royal Society in 2013.

ABSTRACT

Active Matter

Active materials such as bacteria, molecular motors and self-propelled colloids are Nature’s engines. They extract energy from their surroundings at a single particle level and use this to do work. Active matter is becoming an increasingly popular area of research because it provides a testing ground for the ideas of non-equilibrium statistical physics, because of its relevance to the collective behaviour of living creatures, from cells to starlings, and because of its potential in designing nanomachines.

Dense active matter shows mesoscale turbulence, the emergence of chaotic flow structures characterised by high vorticity and

motile topological defects. The chaotic nature of active turbulence means that it is likely to be difficult to harness its energy. Hence it is interesting to consider ways to `tame’ the turbulence, channelling the energy input into coherent flows. This can be done by screening hydrodynamics through confinement or friction, and I will describe flow patterns and defect trajectories in active matter in confined geometries.

Moreover, the ideas of active matter suggest new ways of interpreting cell motility and cell division. In particular recent results indicate that active topological defects may help to regulate turnover in epithelial cell layers and contribute to controlling the structure of bacterial colonies.

Nobel Laureate Professor Rainer Weiss

Massachusetts Institute of Technology, USA

Rainer Weiss (NAS) is a Professor Emeritus at Massachusetts Institute of Technology (MIT). Previously Dr. Weiss served as an assistant physics professor at Tufts University

and has been an adjunct professor at Louisiana State University since 2001. Dr. Weiss is known for his pioneering measurements of the spectrum of the cosmic microwave background radiation, his inventions of the monolithic silicon bolometer and the laser interferometer gravitational wave detector and his roles as a co-founder and an intellectual leader of both the COBE (microwave background) Project and the LIGO (gravitational-wave detection) Project. He has received numerous scientific and group achievement awards from NASA, an MIT excellence in teaching award, the John Simon Guggenheim Memorial Foundation Fellowship, the National Space Club Science Award, the


Medaille de l’ADION Observatoire de Nice, the Gruber Cosmology Prize, and the Einstein Prize of the American Physical Society. Dr. Weiss is a fellow of the American Association for the Advancement of Science, the American Physical Society, The American Academy of Arts and Sciences; and he is a member of the American Astronomical Society, the New York Academy of Sciences, and Sigma Xi. He received his B.S. and Ph.D. in physics from MIT. Dr. Weiss is a member of the NAS and has served on nine NRC committees from 1986 to 2007 including the Committee on NASA Astrophysics Performance Assessment; the Panel on Particle, Nuclear, and Gravitational-wave Astrophysics; and the Task Group on Space Astronomy and Astrophysics.

Sponsored by

ABSTRACT

The beginnings of gravitational wave astronomy

The first detection of gravitational waves was made in September 2015 with the measurement of the coalescence of two ~30 solar mass black holes at a distance of about 1 billion light years from Earth. The talk will provide a review of more recent measurements of black hole events as well as the first detection of the coalescence of two neutron stars and the beginning of multi-messenger astrophysics. The talk will end with a discussion of some prospects for the field.

Professor Michael Wiescher

University of Notre Dame, USA

Michael Wiescher, received his PhD in 1980 at the University of Münster, Germany. After postdoctoral positions at Ohio State University (USA), Caltech (USA), and the University of

Mainz (Germany), he joined the faculty at the University of Notre Dame (USA) to build a program in experimental nuclear astrophysics. In 2003 he founded the Joint Institute for Nuclear Astrophysics (JINA), which is now an international research organization including more than 100 research institutions worldwide. For the period of 2003 to 2014, he served as JINA director. In 2010 he became also the director of the Notre Dame Nuclear Science Laboratory (NSL) at Notre Dame. Wiescher’s research focuses on the experimental and theoretical study of stellar reaction rates for quiescent and explosive stellar environments. More recently Wiescher was instrumental in the installation of CASPAR, the first US deep underground accelerator at Homestake Mine in South Dakota which concentrates on the study of reactions important for stellar helium burning.

In 2003 Wiescher was awarded with the Hans Bethe Prize of the American Physical Society for his work on the rapid proton capture process that drives thermonuclear explosions in accreting binary systems. In 2018 he was awarded the 2018 Prize for Laboratory Astrophysics by the American Astronomical Society for “his leading contributions to the experimental foundation of nuclear astrophysics”. Presently he serves as the Heraeus Guest Professor for Physics at the University of Frankfurt, Germany.

ABSTRACT

Neutron Sources in Stars and the Laboratory

Neutrons play a critical role for the origin of the elements above iron. Next to the r-process in explosive stellar environments, the s-process in quiescent stellar burning is key for the heavy element nucleosynthesis.

Reliable modelling of these processes requires a detailed understanding of stellar neutron sources, the cross section and the impact of hot stellar plasma conditions on the reaction rate. A number of experiments will be presented which aim at the study of the most critical stellar neutron sources at the CASPAR deep underground accelerator


laboratory and the NIF National Ignition Facility for studying these reactions at stellar burning conditions.

Professor Chandralekha Singh

University of Pittsburg, USA

Chandralekha Singh is a professor in the Department of Physics and Astronomy and the Director of the Discipline-based Science Education Research Center at the University of Pittsburgh.

She obtained her Ph.D. in theoretical condensed matter physics from the University of California Santa Barbara and was a postdoctoral fellow at the University of Illinois Urbana Champaign, before joining the University of Pittsburgh. She has been conducting research in physics education for two decades. She was elected to the Presidential-line of the American Association of Physics Teachers and is currently serving as the Vice-President. She was one of the two team leaders of the US team to the 6th International Conference on Women in Physics (ICWIP) in Birmingham UK in 2017 and is an editor of the 6th ICWIP Proceedings. She held the Chair-line of the American Physical Society Forum on Education from 2009-2013 and was the chair of the editorial board of Physical Review Special Topics Physics Education Research from 2010-2013. She has co-organized two physics education research conferences in 2006 and 2007 and was the co-chair of the 2010 Gordon Conference on Physics Research and Education. She co-chaired the first conference which brought together physicists, chemists and engineers from various engineering departments to discuss the future of materials science and engineering education in 2008. She was the co-organizer of the first and third conferences on graduate education in physics in 2008 and 2017 and chaired the second conference on graduate education in physics in 2013. She is a Fellow of the American Physical Society, American

Association of Physics Teachers and the American Association for the Advancement of Science.

ABSTRACTChandralekha Singh1*1 Department of Physics and Astronomy, University of Pittsburgh,

Pittsburgh, PA 15260 United States of America* [email protected]

How to strengthen physics by making it inclusive

The field of physics has historically lacked diversity, and efforts to make it inclusive have been limited in their success. Despite some efforts to encourage women to pursue a career in physics, the percentage of women majoring in physics remains low. There are several frameworks that focus on the dearth of women in physics, which take into account motivational characteristics, e.g., interest in physics, self-efficacy, mindset about intelligence, sense of belonging, and identity as a physicist. We performed a longitudinal analysis of these motivational characteristics of female and male college students in large physics courses along with their performance in those courses. Among other findings, our data suggest that female students had lower physics self-efficacy than male students, even when controlling for performance. Moreover, this self-efficacy gap continued to grow throughout the college introductory physics course sequence. Based upon these findings, we implemented short in-class activities that were designed to improve the inclusivity in the physics courses and address issues related to students’ sense of belonging, self-efficacy and intelligence mindset. We found that female students in physics classes who participated in these activities performed significantly better than those who did not, and they were also less likely to withdraw from the courses.


Professor Susan Scott

Australian National University

Professor Susan Scott is Professor of Theoretical Physics at The Australian National University (ANU). She has a BSc (Hons) majoring in Pure Mathematics from Monash University and a

PhD in Mathematical Physics from The University of Adelaide. As the recipient of a Rhodes Fellowship, she then spent 4 years at The University of Oxford working with the research group led by Prof Sir Roger Penrose, before returning to Australia to take up a research fellowship at the ANU. She has been a faculty member in Physics at the ANU since 1998.

Susan’s research field is general relativity and gravitational physics. She is a leading international expert in the singularity structure of space-time, including the singularities at the heart of black holes as well as cosmological singularities at the beginning and end of the Universe. In 1998 she initiated and led the Australian endeavour in gravitational wave data analysis forming a collaboration with LIGO ultimately leading to participation in the discovery of gravitational waves in 2015. Susan is an author of more than 250 research papers and a definitive book on black holes. She is a fellow of the Australian Academy of Science and the European Academy of Sciences and a former President of the Australasian Society for General Relativity and Gravitation. She is a Chief Investigator with the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav).

Dr Paul Lasky

Monash University

Paul Lasky is a Senior Lecturer and ARC Future Fellow in the School of Physics and Astronomy at Monash University. He earned his PhD from Monash University in 2008, before

being granted an Alexander von Humboldt Fellowship, which he took up at the University of Tuebingen, Germany. He then spent three years as a postdoctoral research fellow at the University of Melbourne, before returning to Monash. Paul’s research field is gravitational physics and high-energy astrophysics. He is an active member of the LIGO Scientific Collaboration that, in 2015, made the first discovery of gravitational waves from colliding black holes. In 2018, Paul won the Australian Academy of Sciences Pawsey medal, recognising outstanding research in physics by scientists up to ten years post PhD.

ABSTRACTSusan Scott1* and Paul Lasky2*1 Australian National University2 Monash University* [email protected]

The Advanced LIG0 gravitational wave detectors have so far undertaken two observing runs, 01 and 02, with spectacular results. At the start of 01 in September 2015 the hundred year quest to directly detect gravitational waves on Earth was quickly realised with the detection of a clear and strong gravitational wave signal coming from the cataclysmic collision of two large black holes in a binary system some 1.3 billion years ago. Towards the end of 02 in August 2017 we achieved the long- anticipated discovery of two orbiting neutron stars in a binary system in the final moments of inspiral leading up to their violent collision. Within 1.7 seconds of the coalescence a gamma-ray burst was detected immediately confirming the long-held hypothesis that neutron star collisions are the progenitors of our almost daily detections of short gamma-ray bursts. Neutron stars are matter, so unlike when two black holes collide, they broadcast electromagnetic as well as gravitational radiation, and the alert sent out by LIG0 caused an avalanche of telescopes and satellites around the world to interrupt their observing schedules to attempt to pinpoint and image the event. This was the birth of the era of multi messenger gravitational wave astronomy.

Since the end of 02, and while upgrading the instruments in preparation for 03, we have had the opportunity to analyse, in greater depth, the data from both 01 and 02 searching for coalescences


of binary systems of black holes and neutron stars. In this talk we will announce the full catalogue of these results from both observing runs and explain the significance of these discoveries for physics.

Professor Monika Ritsch-Marte

Medical University of Innsbruck, Austria

Monika Ritsch-Marte received her M.Sc. in Physics from the University of Innsbruck in 1984 and her PhD in Quantum Optics from the Waikato University in New Zealand (under the

supervision of D.F. Walls) in 1988. After several PostDoc projects (Boulder/Colorado, Milano, Helsinki), and after completing her Habilitation at the Institute of Theoretical Physics in Innsbruck, she accepted the Chair of Biomedical Physics at the Medical University in Innsbruck in 1998 where she founded a Biomedical Optics group. Her current research interests include holographic optical tweezers, digital holographic microscopy and linear and non-linear Raman microscopy. She has received numerous research grants and awards, including an ERC Advanced Grant and the Boltzmann Award of the Austrian Physical Society. She is a member of the Austrian Academy of Science and a Fellow of the Optical Society of America.

ABSTRACT1 Division for Biomedical Physics, Medical University of Innsbruck,

A-6020 Innsbruck, Austria* mo nika.rit [email protected]

In recent years optical wavefront shaping by means of spatial light modulators (SLMs), such as deformable mirrors, digital micro-mirror devices or liquid crystal (LC) panels, has become a powerful tool in Biophotonics [1-2]. “Holographic optical tweezers” are well-known and widespread. But an SLM can also be integrated into optical imaging systems, making the microscope programmable and adaptable with respect to the needs of a specific sample. Iterative search algorithms are used to find the desired phase mask patterns.

A particular strength of the Synthetic Holography [3] approach with programmable phase masks is the possibility to multiplex, which means that one can ‘pack’ several tasks into one computer-generated hologram. One can, for instance, create images which are composed of sub-images belonging to different microscopy modalities, to different depths inside the volumetric sample, or to different parameter settings. Diffractive phase masks normally operate in the modulation range of 0 to 2π. If one relaxes this condition, allowing for multiple-2π phase shifts, several computer- generated holograms can be read out at different wavelengths from one and the same voltage pattern applied to the LC panel. In this way holographically modified imaging (in the visible) can be accommodated in the same phase mask that is used for holographically controlled trapping (in the near-infrared).1. References[1] H. Rubinsztein-Dunlop et al., “Roadmap on structured light”, Journal

of Optics, 19, 013001, 2016.[2] C. Maurer, A. Jesacher, S. Bernet, and M. Ritsch-Marte, “What

spatial light modulators can do for optical microscopy”, Laser & Photonics Reviews 5, 81-101, 2011.

[3] A. Jesacher, and M. Ritsch-Marte, „Synthetic holography in microscopy: opportunities arising from advanced wavefront shaping”, Contemporary Physics, 57, 46-59, 2016.

Professor Jian-Wei Pan

University of Science and Technology of China

Jian-Wei Pan, born on March 11, 1970 in Dongyang, Zhejiang province. He obtained his Bachelor and Master degrees of Theoretical Physics from University of Science and Technology of

China (USTC) in 1992 and 1995. In 1996, he went abroad for studying in Austria, and obtained his Ph.D. degree of Experimental Physics from the University of Vienna in 1999. In 2001, he was appointed as the full professor of physics by USTC. In 2011, he was elected as the academician of Chinese Academy of Sciences (CAS). In 2012, he was elected as the World Academy of Science (TWAS) Fellow. The research of Jian-Wei Pan focuses on quantum optics, quantum information and quantum foundations. As one of pioneers in experimental quantum information science, he has


accomplished a series of profound achievements. Due to his numerous progresses on quantum communication and multi-photon entanglement manipulation, quantum information science has become one of the most rapidly developing fields of physical science in China in recent years.

Sponsored by

ABSTRACT

Breaking the Wall to Quantum Engineering

Quantum information science and technology are emerging and fascinating technologies formed by combining coherent manipulating of individual quantum systems and information technology, which enables secure quantum cryptography (quantum communication), super-fast quantum computing, revealing laws of complex physical systems (quantum simulation), and improving measurement precision (quantum metrology) etc., to beat classical limits. This presentation will highlight a few of our progress along quantum communication, quantum computing, quantum simulation and quantum metrology, based on photons and atoms.

For fundamental aspect, one is led to the conception of quantum entanglement when apply quantum superposition principle to multi-party system. The appeared ‘spooky action at a distance’ phenomena referred by Einstein, is often explained by seemingly reasonable assumptions of “local realism”. The inequalities proposed by John Bell and others provide immediate tests for correctness of quantum mechanics. Many efforts are addressing loophole-free tests of Bell inequalities, which tries to close various loopholes, in which some of loopholes are still needed to be addressed including freedom of choice loophole, the collapse locality loophole. Well, the final test is on-going, many developed ground-breaking technologies for coherent manipulation of quantum systems offers elegant and feasible solutions for satisfying increasing needs of computational power and information security.

Based on state-of-the-art fiber technology and rich fiber resources, we have managed to achieve prevailing quantum communication with realistic devices in real-life situation. This constitutes demonstrations by developing decoy state scheme over 100km firer extending its employment in the metropolitan area network, as well as maintaining Measurement Device Independent QKD (MDI-QKD) over 400km. At the meantime, we are also developing practically useful quantum repeaters that combine entanglement swapping, entanglement purification, efficient and long-lived quantum memory for the ultra-long distance quantum communication. Another complementing route is to attain global quantum communication based on satellite. We have spent the past decade in performing systematic ground tests for satellite-based quantum communications. Our efforts finally ensure a successful launch of the Micius satellite. Three major scientific missions have been finished, which includes achieving QKD between satellite and ground station at thousand kilometer scale, achieving satellite-based entanglement distribution between two ground stations separated by a distance of 1200 km, achieving quantum teleportation from ground to satellite over 1400 km. Very recently, using Micius satellite as a trustful relay, the intercontinental QKD between Beijing and Vienna over a distance of 7600 km has also been realized.

In the areas of optical quantum information processing, we have maintaining a series of technological advances for generating, manipulating and applications of multi-photon entanglement. Over the past decade, we have performed proof-of-principle demonstrations for a number of key quantum algorithms including the Grover’s searching algorithm, Shor’s factoring algorithms, quantum machine learning, topological quantum error correction, and particularly a recent photonic quantum computer to solve the Boson sampling problem.

Future Prospects include building a global quantum communication infrastructure with satellite and fiber networks, quantum computing by employing manipulating coherently more than 50 qubits to exceed the simulating power of


the current best supercomputers and reaching “quantum supremacy”, Bell-test experiment with human-observer at a distance on the order of one light-second.

Professor Willie Padilla

Duke University, USA

Willie Padilla has been in the metamaterials field since 2000, when he co-authored the first paper on negative index materials with Smith. Padilla is particularly well known for his work at

terahertz (THz) frequencies, as well as in the area of active and dynamically controlled metamaterials. While working under a Director’s Postdoctoral Fellowship at Los Alamos National Laboratory, Padilla led efforts to demonstrate dynamic tuning of a semiconductor hybrid metamaterial by photodoping and voltage control. Both of these key experiments are now widely recognized and cited. Padilla’s lab specializes in the THz, infrared, optical and magneto-optic properties of novel materials utilizing various spectroscopic methods, including Fourier transform spectroscopy and ellipsometry. Padilla’s recent interests include tailoring the emissivity of objects with metamaterial coatings, and the use of active metamaterial arrays as components in THz and infrared imaging systems.

ABSTRACT

Exotic Physics with All-Dielectric Metasurfaces

Willie J. Padilla1 *1 Department of Electrical and Computer Engineering, Duke University,

Durham, NC 27708, United States of America* [email protected]

All-dielectric metasurfaces are a useful platform to investigate a myriad of unconventional physical scattering responses ranging from high absorption and Huygens’ reflect arrays to bound-states-in-the-continuum (BIC). We experimentally demonstrate several all-dielectric metasurfaces

which realize: high transmission Huygens’ structures, high absorptive devices for imaging, and dynamic surfaces with optical control. The all-dielectric metasurfaces we explore consists of arrays of high dielectric geometrical shapes, and may support a number of eigenmodes of either odd or even symmetry. [1,2] We show that the geometry of the array may be used to tune the oscillator strength and resonant frequency location of the modes. The physics underlying the nature of the electromagnetic responses is described with temporal coupled mode theory and waveguide analysis.

1. Simulation

The metasurface is simulated using full-wave 3D electromagnetic software, and use the frequency domain solver (finite element method). We use the two-port simulations, where the two ports were set symmetrically with respect to the mid-plane of the unit cell, and periodic boundaries were used on all sides. Eigenvalue simulations are also performed permitting extraction of the modes complex frequency. Metasurfaces may be simulated with and without material loss, which permits us to determine the individual pieces of scattering and dissipative loss in the structures. We use silicon as the base material for our all-dielectric metasurfaces, and – in some studies – use a slight boron doping. The metasurfaces were fabricated by reactive deep ion etching and we use pdms (polydimethylsiloxane) as a support substrate. The all-dielectric metasurfaces are characterized by various methods including a vector network analyser, terahertz time-domain spectroscopy, and Fourier transform spectroscopy.

2. Tunable Metasurfaces

We also demonstrate dynamic control of the amplitude and phase of transmitted light. Two different optical sources are used – a 980nm LED and an ultra-fast titanium sapphire laser producing radiation at a wavelength of 800nm. We obtain a transmitted phase of 120 degrees with transmission modulation of over 99.9%. Theoretical analysis and numerical simulations


coupled with temporal coupled mode theory indicate that the tuning is due to a substantial increase in the material dissipation rate of the odd eigenmode of the structure. This serve to lift the degeneracy of the odd and even eigenmodes, while simultaneously destroying the critical coupled state.

Our all-dielectric metasurface is an ideal platform to investigate unconventional physics in electromagnetic wave absorbing systems. The demonstration of a dynamic all-dielectric structure highlights a new strategy for controlling metasurfaces, and highlights a potential path to achieve reconfigurability for future applications.

Figure 1: Left panel show a photograph of the suspended silicon metasurface array. Middle panel shows a computer rendered depiction of optical photodoping of the array. Right panel show an SEM image of the fabricated silicon metasurface array.

3. References[1] X. Liu, K. Fan, I. V. Shadrivov, W. J. Padilla, “Experimental realization

of a terahertz all-dielectric metasurface absorber,” Opt. Express, vol. 25, p. 191, 2017.

[2] K. Fan, J. Y. Suen, X. Liu, W. J. Padilla, “Degenerate critical coupling in

all-dielectric metasurface absorbers,” Optica, vol. 4, p. 601, 2017.

Professor Teri Odom

Northwestern University, USA

Teri W. Odom is Charles E. and Emma H. Morrison Professor of Chemistry, Professor of Materials Science and Engineering, and Associate Director of the International Institute for

Nanotechnology (IIN) at Northwestern University. She is an expert in designing structured nanoscale materials that exhibit extraordinary size and shape-dependent optical properties. Odom has received numerous honors and awards. Select ones include being named a U.S. Department of Defense Vannevar Bush Faculty

Fellow; a Radcliffe Institute for Advanced Study Fellowship at Harvard University; an NIH Director’s Pioneer Award from the National Institutes of Health; the MRS Outstanding Young Investigator Award; an Alfred P. Sloan Research Fellowship; an NSF CAREER Award; and a David and Lucile Packard Fellowship in Science and Engineering. She is a Fellow of the American Chemical Society, Materials Research Society, and the Royal Society of Chemistry. Odom is the founding Executive Editor of ACS Photonics.

ABSTRACT

Reconfigurable Flat Nanoparticle OpticsTeri W. Odom1

1 Department of Chemistry, Department of Materials Science and Engineering, Northwestern University, Evanston, IL 60208 USA

* [email protected]

Over the past decade, significant progress in controlling light-matter interactions at the nanoscale has been achieved. Most of the advances, however, have relied on fixed systems limited to the as-fabricated or as-synthesized dielectric or metallic nanostructures. This talk will discuss how the ability to program or realize a plasmonic response on demand may address key challenges in future nanoscale optics. We will highlight how the fabrication and scalability of responsive nano-optical flat optics can be used in diverse applications from stretchable nano-lasing to reconfigurable lensing and imaging.

Professor Thomas Krauss

University of York, UK

Prof Thomas Krauss is Professor of Photonics at the University of York, UK. He is interested in fundamental and applied concepts of light-matter interaction in photonic nanostructures and he has

led a number of EU and EPSRC projects in various aspects of photonic crystal devices, such as slow light, optical interconnects and, more recently, novel photonic concepts for biosensing. He has published 300 refereed journal articles and 6 patents. Prof Krauss is a Fellow of the Institute of Physics, the Royal Society of


Edinburgh and the Optical Society. In 2015, he was awarded a Royal Society Wolfson Merit Award.

ABSTRACT

Photonic Crystals and Nanostructures – Phoenix of Photonics?Thomas F Krauss Department of Physics, University of York, York YO10 5DD, [email protected]

Photonic crystals were invented in the late 1980’s as a tool for exercising spontaneous emission control. By introducing the language of solid state physics into photonics, they have transformed the way we think about diffractive optics. As a result, there was much excitement and a lot of new activity emerged in the 1990’s and 2000’s. Photonic crystals were eventually replaced by other “hot topics”, yet many of these topics are actually founded on similar principles. In particular, the Bloch mode formalism, which is a key feature of the bandstructure description of the photonic crystal paradigm, underpins many modern research areas, including metalenses, label-free resonant imaging and nanostructures for light trapping.

The idea of Bloch modes dates back to 1929, when they were first described in the context of electron wavefunctions in crystal lattices [1]. Bloch modes can be understood as interference patterns arising from multiply Bragg-scattered waves. Formally, they are described as follows,

So, a Bloch mode describes the interference pattern between a plane wave with wavevector k and the sum over all possible lattice vectors G.

1. Metasurfaces

Metasurfaces are nanostructured thin films that can imprint an arbitrary phase profile onto a given beam; they can do this by creating localised resonances or by adding specific wavevectors to the beam, thereby invoking the Bloch formalism. Metalenses in particular open new possibilities in miniaturised optical systems with the smartphone market in mind [2], especially since high performance silicon-based structures have now

also been demonstrated in the visible [3, 4].

Figure 1. Illustration of a silicon metalens with ultrahigh numerical aperture [4].

2. Sensing and Imaging

Metasurfaces have now also entered the sensing domain; sensing often relies on spectral information, be it via fluorescence, absorption spectroscopy or by tracking resonances. By recognising the equivalence of wavelength

and lattice constant that is inherent in the Bloch mode formalism, it is possible to translate spectral information into spatial information. This ability has been demonstrated with the chirped guided mode resonance approach [5] and the “molecular barcoding” method [6]. The related technique of resonant imaging tracks resonances locally to extract information on e.g. cell adhesion [7] or the secretion of proteins [8], all in real time and with the possibility to use clinical samples because of the label-free nature of the process.

3. Light trapping

The final example comes from yet another domain, namely light trapping, which is used to enhance the absorption in thin film solar cells. By exploiting Bloch modes and manipulating their respective phases, we can selectively excite the modes that most effectively contribute to the absorption of sunlight [9].

4. References[1] F. Bloch, “Über die Quantenmechanik von Elektronen in

Kristallgittern”, Zeitschrift f. Physik 52, pp. 555-600, 1929. [2] M. Khorasaninejad, W.T. Chen, R.C. Devlin, J. Oh, A. Zhu, and F. Capasso, ”Metalenses at visible wavelengths: Diffraction-limited focusing and subwavelength resolution imaging” Science 352, pp.1190−1194, 2016.

[3] Z. Zhou, J. Li, R. Su et al., “Efficient Silicon Metasurfaces for Visible Light”, ACS Photonics 4, pp. 544-551, 2017.

[4] H. Liang, Q. Lin, X. Xie et al., “Ultrahigh numerical aperture metalens

23rd Australian Institute of Physics Congress – SPONSORSHIP & EXHIBITION PROSPECTUS24

at visible wavelengths, Nano Lett. 18, pp. 4460–4466, 2018.[5] G. Triggs, Y. Wang, C. Reardon, M. Fischer, G.J.O. Evans and T.F.

Krauss, “Chirped guided-mode resonance biosensor”, Optica 4, pp.229-234, 2017.

[6] A. Tittl, A. Leitis, M. Liu et al., “Imaging-based molecular barcoding with pixelated dielectric metasurfaces” Science 360, pp. 1105–1109, 2018.

[7] Y. Zhuo, J.S. Choi, T. Marin, H. Yu, B.A. Harley and B.T. Cunningham, “Quantitative analysis of focal adhesion dynamics using photonic resonator outcoupler microscopy (PROM)”. Light Sci. Appl. 7, Art. 9, 2018.

[8] J. Juan-Colás, I. Hitchcock, M. Coles, S. Johnson and T.F. Krauss, “Quantifying single cell secretion in real time using resonant hyperspectral imaging” unpublished.

[9] E.R. Martins, J. Li, Y. Liu, V. Depauw, J. Zhou and T.F. Krauss, “Deterministic quasi-random nanostructures for photon control” Nature Communications 4, Art. 2665, 2013.

Professor Garth Illingworth

UC Santa Crus/Lick Observatory

Garth Illingworth is a Professor at the University of California, Santa Cruz. He was a Miller Fellow at UC Berkeley, the Deputy-Director of the Space Telescope Science Institute, and in 2010 was

awarded an honorary Doctor of Science degree at the University of Western Australia. He is the recipient of the 2016 American Astronomical Society Lancelot M. Berkeley New York Community Trust Prize for his work on The most-distant galaxies viewed with Hubble.

He has been exploring for the earliest galaxies in the first 1-2 billion years of the Universe with the world’s most powerful telescopes, the Hubble and Spitzer space telescopes and the Keck telescope on Mauna Kea. Central to his research has been to use Hubble to look back through 96% of all time to find and measure incredibly faint, young galaxies that are the seeds that have grown into galaxies today, like our Milky Way.

A recent highlight of this research is the discovery of the most distant, and earliest, galaxy ever seen, just 400 million years after the Big Bang at redshift z=11.1. The publications from this research on the most distant and earliest galaxies, with an international team of scientists, have consistently been among the most highly

cited papers on galaxies in the early universe (see firstgalaxies.org). The latest results on the sizes of distant galaxies and on the star formation rate density at z~10, combined with the latest Planck results that indicate that reionization began around redshift z~10, have significant implications for the detectability of the “first galaxies” with the James Webb Space Telescope (JWST). He recently gave the Lancelot M. Berkeley Prize plenary talk at the 2017 meeting of the American Astronomical Society.

ABSTRACT

Garth Illingworth Department of Astronomy University of California Santa Cruz

The Hubble Space Telescope has revolutionized the discovery and study of the earliest galaxies through its exploration of the Universe in the first billion years after the Big Bang. I will discuss what we have learned about galaxies during that epoch at redshift z>6 from the remarkable Hubble and Spitzer Space Telescope imaging surveys, as well as detections of gravitationally-lensed galaxies behind massive clusters of galaxies. Lensing clusters provide extraordinary opportunities for characterizing the faintest earliest galaxies, but also present extraordinary challenges. Analysis of early galaxies found in deep cluster images reveal compact star-forming regions that, remarkably, can be as small as today’s globular clusters and dwarf galaxies.

The results from deep surveys with Hubble, combined with the recent results on the Cosmic Microwave Background from the Planck space telescope, indicate that galaxies dominated the UV ionizing flux that reionized the Universe. One of the greatest surprises came from the Hubble discovery of very luminous galaxies at redshifts z~11 to z~8, just 400 to 650 million years after the Big Bang. Hubble and Spitzer have encroached on James Webb Space Telescope (JWST) territory by looking back through 97% of all time to confirm a z~11.1 galaxy. This is far beyond what we ever expected Hubble and Spitzer could do.

Twenty years of astonishing progress with Hubble and Spitzer leave me looking to JWST to provide


even more remarkable exploration of the realm of the first galaxies. I will give an update on JWST’s progress towards its launch, and then I will discuss how the latest Hubble and Spitzer results on the sizes of star-forming regions in distant galaxies, on the star formation rate at redshift z~10, and from Planck indicating that reionization began around z~10, together have significant implications for the detectability of the “first galaxies” with JWST.

Maureen Frank

Diversity and Equity Group in Australian Physics Keynote

Leading international business woman – former head of Mergers and Acquisitions for Aon in UK and Australia, Telstra Business Woman of the Year,

BRW Rising Star and founder of emberin 10 years ago.Diversity and inclusion expert – Maureen, with her ROI obsession has established over a dozen diversity councils in major organisations (most of which were the executive team), personally coached CEO’s on their journey and supported her client to achieve results, including supporting a number of organisations increase the number of women in senior leadership in record time: a telco (from 6% to 31% in 2 years), a mining company (from 8% to 23% in 2 years), a bank (from 11% to 33% in 3 years), a waste management business (from 8% to 19% in 1 year) and many more examples.

Speaker, entertainer and thought leader – she has spoken at conferences in five continents around the world.Bestselling author, writer and creator – her books, publications and programs have been used by over 50,000 people worldwide. Global Award winner – her clients have won multiple awards, acknowledging emberin as the cornerstone of success, including two global

Catalyst Awards in New York. Pioneer and challenger – Maureen pioneered the scalable engagement of men in the diversity and inclusion conversation globally, supported founding the Male Champions of Change (CEO’s of major companies supporting gender diversity) and engages CEO’s and leaders every week in understanding how inclusion enables not just diversity – but also engagement, innovation and collaboration.

Tara Fortier

National Institute of Standards and Technology, USA

Dr. Tara Fortier is a Project Leader at the National Institute of Standards and Technology and serves as Graduate Faculty at the University of Colorado, Boulder. Her research is focused on the development and application of optical frequency combs for high precision atomic clock comparisons and ultra low-noise microwave generation. She received her Ph.D at JILA/ University of Colorado on the development of phase-stabilized ultra-fast lasers for quantum coherent control experiments. As a Postdoctoral Director’s Fellow at Los Alamos National Laboratory she performed optical atomic clock comparisons as a means to search for time variation of fundamental constants and violations of physical laws. She was awarded the 2009 European Time and Frequency Forum Young Scientist Award for her contributions to optical frequency comb development, was a successful champion in the DARPA PULSE Program, and has served as the government evaluator for the DARPA EPHI and STOIC programs. Finally, Dr. Fortier serves on the NIST board of directors for Women in STEM and is committed to serving

and advancing the representation of women and minorities in physics and photonics.


BIO/ABSTRACT

Optical networks and clock comparisons at the 18th-decimal place

Tara Michele FortierNational Institute of Standards and Technology, 325 Broadway MS 847,

Boulder CO 80302 USADepartment of Physics, University of Colorado, Boulder CO 80309 USA* [email protected]

The generation of frequency references from quantum mechanical systems have been instrumental in enabling a timing stability and resolution that are unattainable using classical architectures. Atomic clocks, which produce frequency in a deterministic way, are used as precision time-keepers in atomic time-scales, as frequency references in precision physical measurements, and are necessary for positioning, timing and synchronization in global networks [1]. Atomic clock transition frequencies are now being reported with an uncertainties approaching 1 part in 10^18, achieved by harnessing the decreased uncertainty and instability of optical as opposed to microwave transitions [2]. This exquisite resolution and the transition frequencies’ dependence on physical laws and fundamental constants make atomic clocks elegant systems for tests of fundamental physics. In this talk I will discuss the results from recent measurement campaigns between the National Institute of Standards and Technology and the University of Colorado to compare optical atomic clock frequencies to the 18th digit. I will also describe the optical networks that connect and facilitate the precision measurements and describe how the clock network is being used for searches of ultra-light dark matter [3].

1. References[1] A. Bauch, “Caesium atomic clocks: function, performance and

applications,” Meas. Sci. Technol. 14, pp. 1159-1173 (2003).[2] W. F. McGrew et al, “Atomic clock performance beyond the geodetic

limit,” arXiv:1807.1128 arXiv:1807.1128, July 2018.[3] A. Arvanitaki, J. Huang, J. and K. Van Tilburg, “Searching for dilaton

dark matter with atomic clocks,” Phys. Rev. D 91, 015015 (2015).

Professor Philippa Browning

University of Manchester, UK

Philippa Browning is a Professor at the Jodrell Bank Centre for Astrophysics at the University of Manchester in the UK. Following a degree in Mathematics at Cambridge and a PhD at St

Andrews, she became the first woman appointed to lecture in Physics at Manchester. Her research is concerned with the mysterious fourth state of matter – plasma. She uses mathematical modelling and computer simulation to understand the complex interactions between plasmas and magnetic fields, with application both to the atmosphere of the Sun and to the generation of energy by nuclear fusion. A main focus of her research is to exploit synergies between these apparently very different fields. Philippa enjoys teaching undergraduates and postgraduates in physics and astronomy, conveying the excitement of the subject to the next generation. She is also passionate about communicating to the general public and is involved in many public talks and events. She was awarded the Chapman Medal of the Royal Astronomical Society in 2016.

Sponsored by

ABSTRACT

Self organisation by magnetic reconnection in solar and fusion plasmas

Philippa K Browning1

1 Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Manchester M13 9PL, UK

* [email protected]

Magnetised plasmas in the laboratory and astrophysics are complex systems, and the concept of “self-organisation” provides a powerful tool for understanding and predicting many phenomena. Magnetic reconnection is a process which reconfigures the magnetic field topology and allows rapid release of free magnetic energy. A magnetised plasma undergoing turbulent


reconnection is predicted to relax to a state of minimum magnetic energy whilst conserving magnetic helicity [1]. Recent advances in relaxation theory shed new light on how solar flares are triggered and accelerate charged particles to high energies, and how the solar corona is heated to high temperatures, as well as how spherical tokamak plasmas can be formed, and the nonlinear development of instabilities in the edge of tokamaks. This talk focuses on reconnection and self-organisation in twisted magnetic flux ropes, which are fundamental structures in fusion and astrophysical plasmas.

1. Relaxation and reconnection in twisted flux ropes: solar flares and tokamak edge-localised modes

Magnetic energy may be stored in twisted magnetic flux ropes in the solar corona, and the release of this stored energy may result in large-scale solar flares or smaller “nanoflares” associated with heating of the solar corona. The ideal kink instability in a twisted flux rope triggers relaxation, through reconnection in fragmented current sheets during the nonlinear phase of the instability.

This results in plasma heating and acceleration of non-thermal particles as the magnetic field relaxes to a lower energy state [2]. Building on idealised models of relaxation in cylindrical flux ropes, a realistic model of an unstable twisted coronal loop is developed, representing a confined solar flare [3]. Exploiting a combination of 3D magnetohydrodynamic (MHD) simulations and test- particle modelling, the observational signatures of both thermal plasma and energetic non-thermal particles can be predicted, providing a means to detect twisted magnetic fields through X-ray and radio observations. Similarly, current-driven instabilities during Edge Localised Modes in tokamaks may trigger localised relaxation of the edge plasma, and a relaxation-based model of this process explains some surprising experimental observations [4].

2. Self organisation of multiple flux ropes in spherical tokamaks and the solar corona

Two or more twisted flux ropes may interact and merge, leading to magnetic self-organisation. Models of merging plasma flux ropes using Hall-MHD simulations and analytical relaxation theory provide good agreement with experimental observations of merging-compression formation in the MAST spherical tokamak [5]. An avalanche of heating events in stable twisted flux ropes may be triggered by instability of a single unstable flux rope, with implications for solar coronal heating. For the first time, such a heating avalanche, predicted by cellular automaton models, is demonstrated from first principles by 3D MHD simulations [6]. This may be described through a relaxation model, showing that multiple flux ropes self- organise into a large-scale coherent structure [7]. Recently, this model has been extended to consider energetic particles and external driving.

3. References[1] J.B. Taylor, “Relaxation of toroidal plasma and generation of reverse

magnetic fields”, Phys. Rev. Lett., vol. 33, pp. 1139-1141, 1974.[2] P.K. Browning and R. Van der Linden, “Solar coronal heating by

relaxation events”, Astron. Astrophys., vol. 400, pp. 355-367, 2003.[3] R.F. Pinto, M. Gordovskyy, P.K. Browning and N.Vilmer, “Thermal and

non-thermal emission from reconnecting coronal loops”, Astron. Astrophys., vol 585, A159, 2016.

[4] Y. Liang, C. Gimblett, P.K. Browning et al, “Multi- resonance effect in Type-I Edge Localised Mode control with low-n fields on JET”, Phys. Rev. Lett., vol. 105, 065001, 2010

[5] P.K. Browning, “Two fluid and MHD modelling of magnetic reconnection in the MAST spherical tokamak and the solar corona”, Plas. Phys. Cont. Fus. Res., vol. 58, 014041, 2016.

[6] A.W. Hood, P. Cargill, P.K. Browning and K.V. Tam, “An MHD avalanche in a multi-threaded coronal loop”, Astrophys. J., vol. 817, 5, 2016.

[7] A Hussain, P.K. Browning and A.W. Hood, “A relaxation model of coronal heating in multiple interacting flux ropes”, Astron. Astrophys,, vol. 600, A5, 2017.

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of J

ian-

wei

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Qua

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Intro

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and

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1035

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Hal

l, Un

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Cong

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Cod

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Our c

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Gra

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Nuc

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1245

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1330

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NCUR

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SES

SION

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Sess

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Gra

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2B -

AIP

Nuc

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artic

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2C -

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CM

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2D -

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ATM

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1145

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0Ax

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axim

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isor

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st

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oder

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inte

nsiti

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Har

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igh

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mitt

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1200

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crea

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char

acte

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of o

ptic

al

defe

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to a

pplic

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bi

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chin

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clo

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olf

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and

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cs

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enne

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s

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on

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ron

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r Int

egra

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tum

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Noah

Men

dels

on

1215

-123

0Na

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mon

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neto

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hani

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f Hex

agon

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Mag

net C

o4Nb

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with

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In-p

lane

Ani

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Guoc

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eng

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Ed

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rras

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onfin

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the

Forc

e of

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ht

Xin

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Nonr

ecip

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qua

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sel

optic

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am fo

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ppin

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rticl

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air

Seba

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vin

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odel

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agin

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plic

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Dhie

ndra

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1230

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1245

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athe

mat

ical

Phy

sics

in A

ustra

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Arts

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.62]


1330

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NCUR

RENT

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5

Sess

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5A -

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Com

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5B -

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atte

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IP C

MM

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5E -

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duca

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and

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5G -

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Arts

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.59]

Univ

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Arts

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uild

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Room

6 [G

.62]

1330

-134

5Co

nstra

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orph

olog

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ga

mm

a-ra

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gr

avita

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gam

ma

rays

Er

ic T

hran

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Sear

ch fo

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atte

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the

ATLA

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LHC

Fr

ance

sca

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New

fron

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tom

pr

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Julie

Cai

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Optic

al n

etw

orks

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cl

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com

paris

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at

the

18th

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pla

ce

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For

tier

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rans

port

of

phon

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and

phot

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Flor

ian

Mar

quar

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valu

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teac

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el

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Jan-

Phili

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Phot

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twor

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Ian

Wal

msl

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Com

putin

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atom

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cale

with

qu

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m d

ots

Konr

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alus

Teac

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Nex

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sics

Ed

ucat

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ur

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forc

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phy

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cent

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1330

-150

013

45-1

400

The

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Infla

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sea

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avita

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ith

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Sout

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Chris

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hard

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Mirr

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ark

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oot

1400

-141

5De

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who

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Ro

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mith

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sear

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atte

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SABR

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Ibtih

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ahm

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Mac

rosc

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Kel

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Prob

e M

icro

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in B

aiki

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Ultra

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pole

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Jo

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mot

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obj

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M

att W

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Sing

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pin

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abric

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devic

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silic

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Ludw

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ranz

1415

-143

0Un

veilin

g th

e vio

lent

Un

ivers

e w

ith

grav

itatio

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ave

astro

nom

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ic H

owel

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Dire

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nal D

ark

Mat

ter

Dete

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Theo

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001)

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w

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pagn

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Evap

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of a

gia

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quan

tum

vor

tex

Yauh

en S

achk

ou

Pale

olith

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aero

dyna

mic

s:

the

stra

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Tim

o Ni

emin

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Redu

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Two-

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1430

-144

5A

sear

ch fo

r con

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us

grav

itatio

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aves

fro

m H

.E.S

.S. s

ourc

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sha

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Radi

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arac

teris

atio

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hi

gh-p

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dar

k m

atte

r de

tect

or m

ater

ials

us

ing

Acce

lera

tor M

ass

Spec

trom

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An

ton

Wal

lner

Met

al C

lust

ers

on S

urfa

ces

for

Phot

ocat

alys

is

Appl

icat

ions

Gu

nthe

r And

erss

on

Gian

t Spi

n Sq

ueez

ing

for m

etro

logy

usi

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Geom

etric

Qua

ntum

Ga

tes

Jaso

n Tw

amle

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Inte

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vers

ion

of

finite

-size

qua

ntum

re

sour

ces

Kam

il Ko

rzek

wa

Beyo

nd F

lippe

d!

Chal

leng

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ased

le

arni

ng in

1st

yea

r Ph

ysic

s an

d Ch

emis

try

Jam

ie Q

uint

on

Inte

grat

ed d

evic

e fo

r Co

ntin

uous

Var

iabl

e qu

antu

m o

ptic

s M

irko

Lobi

no

Mic

rose

cond

spi

n qu

bit r

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ith a

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el

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n tra

nsis

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Dani

el K

eith

1445

-150

0In

ferri

ng p

opul

atio

n pr

oper

ties

of b

inar

y ne

utro

n st

ars

with

gr

avita

tiona

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es

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jiang

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Broa

dban

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tect

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of A

xion

Win

d us

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Mag

nons

Gr

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Plas

mon

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of t

he E

lect

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Inel

astic

Mea

n Fr

ee P

ath,

en

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loss

func

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, for

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nerg

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Chris

toph

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hant

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Com

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bidi

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lock

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erre

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nom

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real

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Man

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umar

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Surv

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s in

a

diss

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drive

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om o

ptic

s sy

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gr

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Mik

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And

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Isot

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ally

Pure

Si

lcon

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Whi

sper

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Galle

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ode

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Hos

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Na

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Lin

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pin

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mbl

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Mic

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1500

-151

5De

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in

grap

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Ro

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M

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1500

-153

0Af

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Unive

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1530

-174

5CO

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SES

SION

6

Sess

ion:

6A -

AIP

Gra

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aves

& R

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6B

- A

IP N

ucle

ar &

Pa

rtic

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hysi

cs

6C -

AIP

Pla

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Phys

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6D -

AIP

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6E- A

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sion

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ptic

al &

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Arts

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Build

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Build

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Naiy

in W

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Phys

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Build

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215

Le

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aria

Par

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Teac

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Sess

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AIP

Ast

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Bio

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Phys

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Build

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Ast

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ahl

Scie

ntifi

c W

ritin

g W

orks

hop

The

Secr

ets

of S

cien

tific

Publ

ishi

ng

Igor

Aha

rano

vich

1330

-150

0

1400

-141

5M

ulti-

mes

seng

er

astro

nom

y in

the

Grav

itatio

nal W

ave

Dete

ctio

n Er

a M

atth

ew B

aile

s

The

impa

ct o

f 3D

surfa

ce

curv

atur

e on

tiss

ue g

row

th

and

orga

niza

tion

Seba

stia

n Eh

rig

Syst

emat

ic s

tudi

es

on Z

dep

ende

nce

of

extre

me

ultra

viole

t and

so

ft X-

ray

spec

tra u

sing

hi

gh-t

empe

ratu

re fu

sion

pl

asm

as

Chih

iro S

uzuk

i

Prac

tical

Met

amat

eria

ls

Fabr

icat

ed b

y Fi

bre

Draw

ing

Sim

on F

lem

ing

A hy

brid

qua

ntum

mem

ory

for m

icro

wav

e ph

oton

s M

ykha

ilo S

avyt

skyi

Publ

ic a

nd T

each

er

Resp

onse

to E

inst

eini

an

Phys

ics

in S

choo

ls

Alex

Fop

poli

Rare

-ear

th g

lass

coa

tings

on

exp

osed

cor

e fib

res

for h

igh

spat

ial r

esol

utio

n te

mpe

ratu

re s

ensi

ng

Dani

el S

tavr

evsk

i

Tem

pera

ture

effe

cts

on

mic

roca

ntile

ver b

ased

hy

drog

en s

enso

rs

Jega

Thi

san

Guru

sam

y

1415

-143

0Al

ice

in W

onde

rland

: How

to

und

erst

and

Dem

entia

fro

m fu

ndam

enta

l X-r

ay

Optic

s Ch

risto

pher

Cha

ntle

r

Dyna

mic

ally

Switc

habl

e Co

lloid

al A

u Na

noro

d Pl

asm

onic

Pixe

ls

Nich

olas

Gre

ybus

h

Exch

ange

-bas

ed 2

-qub

it lo

gic

gate

s w

ith d

onor

s in

silic

on

Mat

eusz

Mad

zik

The

new

HSC

phy

sics

sy

llabu

s –

wha

t sup

port

do te

ache

rs n

eed?

Lo

rna

Jarr

ett

Mul

ti-w

avel

engt

h th

ird

harm

onic

gen

erat

ion

usin

g ex

pose

d-co

re

mic

rost

ruct

ured

opt

ical

fib

re

Step

hen

War

ren-

Smith

A Ne

w A

ppro

ach

to

Mod

ellin

g th

e Co

here

nce

of O

ptic

al F

eedb

ack

in

Dyna

mic

al S

emic

ondu

ctor

La

ser S

yste

ms

Deb

Kane

1430

-144

5Po

sitro

n an

nihi

latio

n in

the

Milk

y W

ay

Fion

a He

len

Pant

her

Brid

ging

the

shor

t and

lo

ng te

rm m

echa

nics

of

arti

cula

r car

tilag

e ex

trace

llula

r mat

rix

Bruc

e Ga

rdin

er

Ener

getic

par

ticle

driv

en

mod

e ac

tivity

: adv

ance

s in

un

ders

tand

ing

from

line

ar

thro

ugh

hard

non

linea

r re

gim

e M

atth

ew H

ole

Real

izatio

n of

Com

plex

-Va

lued

Bire

fring

ence

with

Di

elec

tric

Met

asur

face

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aun

Lung

Fide

lity

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r tw

o qu

bit g

ates

in s

ilicon

W

iste

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Embe

ddin

g hi

gh s

choo

l Ph

ysic

s te

ache

rs w

ithin

th

e un

ivers

ity s

yste

m –

re

flect

ions

by

a ‘V

isiti

ng

Teac

hing

Fel

low

’ Je

ssic

a Bu

dden

SPDC

spe

ctro

scop

y on

a

lithi

um n

ioba

te c

hip

Alex

ande

r Sol

ntse

v

Focu

sed

elec

tron

beam

in

duce

d pr

oces

sing

for

nano

phot

onic

app

licat

ions

Ja

mes

Bis

hop

1445

-150

0Ch

arac

teris

ing

“Hot

Ju

pite

r" E

xopl

anet

s Gr

aem

e M

elvi

lle

Influ

ence

of h

ydra

tion

in m

olec

ular

dyn

amic

s si

mul

atio

ns o

f DOP

C m

embr

anes

with

glyc

erol

an

d DM

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Chris

toph

er M

alaj

czuk

Mou

rou’

s ve

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xtre

me

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Lase

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for

Non-

Ther

mal

Las

er B

oron

Fu

sion

Rea

ctor

for C

lean

El

ectri

city

like

Nuc

lear

Fi

ssio

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ra

Mee

ting

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chal

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ccur

ate

dim

ensi

onal

m

easu

rem

ents

at t

he

nano

scal

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kir B

abic

Fide

lity

benc

hmar

ks fo

r tw

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ates

in s

ilicon

St

ephe

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rtle

tt

Gene

ral r

elat

ivity

in u

pper

se

cond

ary

scho

ol: D

esig

n an

d ev

alua

tion

of a

n on

line

lear

ning

env

ironm

ent

usin

g th

e m

odel

of

educ

atio

nal r

econ

stru

ctio

n M

agda

lena

Ker

stin

g

Ther

mal

ly dr

awn

polyu

reth

ane

optic

al fi

bres

fo

r sen

sing

app

licat

ions

Si

mon

Fle

min

g

Com

paris

on o

f Si,

SiGe

an

d Ga

As p

hoto

volta

ic

mic

roce

lls fo

r pow

er-

over

-fibr

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even

Hin

ckle

y

1500

-153

0Af

tern

oon

Tea

Banq

uet H

all,

Unive

rsity

Clu

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1530

-174

5CO

NCUR

RENT

SES

SION

9

Sess

ion:

9A -

AIP

– M

edic

al

Phys

ics

Com

bine

d w

ith A

IP -

Syn

chro

tron

Sc

ienc

e, S

catte

ring,

M

icro

scop

y, Im

agin

g

9B -

Foc

us S

essi

on –

Da

rk M

atte

r Det

ectio

n 9C

- A

IP P

lasm

a Ph

ysic

s 9D

- F

ocus

Ses

sion

–

Nano

stru

ctur

es &

M

etam

ater

ials

9E -

AIP

ATM

OP

9F -

Foc

us S

essi

on

– Op

tical

& Q

uant

um

Bio-

Sens

ing

9G -

AOS

/ACO

FT

9H -

Foc

us S

essi

on –

50

year

s of

Bic

ontin

uous

Cu

bic

Phas

es

Educ

atio

n fo

r Phy

sics

an

d Re

late

d Di

scip

lines

–

Addi

tiona

l

Topi

c:Sc

atte

ring

Biop

hoto

nics

& p

hysi

olog

y

Chai

r:Ri

char

d Ga

rret

t &

Azin

Aza

diEl

isab

etta

Bar

berio

Snez

harn

a I.

Abar

zhi

Ann

Robe

rts

& M

ohse

n Ra

hman

iJu

lian

Bere

ngut

Davi

d Si

mps

onJi

awen

Li

Bodo

Wilt

s Ge

rd S

chro

der-

Turk

Room

:Ph

ysic

s Bu

ildin

g Cl

ews

Lect

ure

Thea

tre

[2.4

3]

Univ

ersi

ty C

lub

Audi

toriu

mAr

ts B

uild

ing

Room

5 [G

.61]

Arts

Bui

ldin

g Ro

om 8

[1.6

0]Ar

ts B

uild

ing

Fox

Lect

ure

Thea

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[G.5

9]

Arts

Bui

ldin

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stin

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The

atre

[1

.59]

Arts

Bui

ldin

g Ro

om 9

[1.6

1]Ph

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s Bu

ildin

g Ro

ss L

ectu

re T

heat

re

[G.4

1]

Phys

ics

Build

ing

Room

215

Lec

ture

Th

eatr

e

1530

-154

5Us

e of

nov

el p

ixela

ted

sem

icon

duct

or d

etec

tors

in

Tar

gete

d Al

pha

Ther

apy

Eva

Beza

k

Heat

ing

up N

eutro

n St

ars

with

Dar

k M

atte

r Ni

cole

Bel

l

Mat

eria

ls u

nder

ext

rem

e pl

asm

a en

viron

men

ts:

Effic

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one

-ste

p pl

asm

a sy

nthe

sis

of s

urfa

ce

nano

stru

ctur

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Corm

ac C

orr

Thre

e-Di

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Tuni

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f the

Nea

r-Fi

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in C

oupl

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etal

Na

nost

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Al

ison

Fun

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Appl

icat

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of t

he

conv

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lose

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plin

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: fro

m a

ntih

ydro

gen

form

atio

n th

roug

h to

co

llisio

ns w

ith m

olec

ular

ta

rget

s

Igor

Bra

y

Nano

scal

e Bi

oPho

toni

cs:

usin

g na

nom

ater

ials

and

lig

ht to

und

erst

and

the

inne

r wor

king

s of

the

body

Br

ant G

ibso

n

Farm

s an

d Ph

oton

ics:

La

sers

, Milk

and

Spe

rm

Sorti

ng

Cath

er S

imps

on

Theo

ry a

nd e

xper

imen

ts

of n

ovel

pol

ycon

tinuo

us

liqui

d cr

ysta

ls

Step

hen

Hyde

Teac

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Nex

us:

Evol

ving

Phy

sics

Ed

ucat

ion

in O

ur

Scho

ols

(W

orks

hop

3)

Pres

ente

r: Pr

of D

avid

Bl

air (

UWA)

Ein

stei

nian

Ph

ysic

s15

30-1

700

1545

-160

0

1600

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5Ki

dney

nep

hron

s an

d po

docy

tes

- to

war

ds in

viv

o im

agin

g an

d im

prov

ed

clin

ical

man

agem

ent

John

Ber

tram

Sear

chin

g fo

r fuz

zy d

ark

mat

ter i

n th

e Ga

laxy

with

Pa

rkes

Pul

sar T

imin

g Ar

ray

Xing

jiang

Zhu

New

exp

erim

enta

l find

ings

of

non

-loca

l tra

nspo

rt in

J-

TEXT

and

KST

AR

Yuej

iang

Shi

Synt

hetic

opt

ical

no

nlin

earit

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die

lect

ric

and

plas

mon

ic

nano

susp

ensi

ons

Zhig

ang

Chen

Vibr

atio

nally

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olve

d el

ectro

n-im

pact

exc

itatio

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mol

ecul

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ydro

gen

Liam

Sca

rlett

Dyna

mic

qua

ntum

sen

sing

of

par

amag

netic

spe

cies

us

ing

nitro

gen-

vaca

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cent

re

Mel

issa

Mat

her

A m

inim

um o

ptic

al

fibre

set

up fo

r RED

OX

mea

sure

men

ts

Wen

Qi Z

hang

Broa

dban

d ci

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ar

dich

rois

m in

met

allic

gy

roid

mic

ro-s

truct

ures

Benj

amin

Cum

min

g

1615

-163

0Se

arch

for Q

CD A

xion

Dark

Mat

ter w

ith R

adio

Te

lesc

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Pe

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uinn

Auge

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con

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spec

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of m

edic

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radi

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125

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Pi E

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Ligh

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Do

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Spi

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Silk

Opt

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Mic

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De

b Ka

ne

Self-

asse

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hex

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to in

finite

bic

ontin

uous

cu

bic

polyh

edra

To

mon

ari D

oter

a

1630

-164

5A

call

to a

rms:

eng

agin

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ists

in th

e fig

ht

agai

nst c

ance

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artin

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rt

Dete

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cha

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atio

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r the

SAB

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outh

dar

k m

atte

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Greg

Lan

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Parti

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mot

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in 3

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HD

equi

libria

ver

sus

rela

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stat

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Davi

d Pf

effe

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Effe

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f Sha

pe a

nd

Aggr

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in P

lasm

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Ra

ndom

Las

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Judi

th D

awes

Trea

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elec

tron

and

posi

tron

trans

port

thro

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liqui

ds fr

om fi

rst p

rinci

ples

Da

nny

Cock

s

Smar

t mic

rosc

opy:

An

adap

tive

way

of s

cann

ing

Nico

las

Mau

rany

apin

Trac

king

and

man

ipul

atin

g th

e fis

h in

ner e

ar to

un

ders

tand

ing

soun

d lo

caliz

atio

n M

icha

el T

aylo

r

Orig

in o

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irror

Sym

met

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reak

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in B

icon

tinuo

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ubic

and

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n-cu

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Phas

es

Gora

n Un

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1645

-170

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w D

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Opt

ics

for

Soft

X-ra

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grap

hy

Alal

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min

zade

h

Ioni

satio

n si

gnat

ures

of

sub-

GeV

dark

mat

ter

due

to a

bsor

ptio

n an

d sc

atte

ring

of e

lect

rons

Benj

amin

Rob

erts

Plas

men

e: a

met

asur

face

pe

rfect

abs

orbe

r Da

niel

Gom

ez

Conv

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nt c

lose

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plin

g ap

proa

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pro

ton

collis

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with

hel

ium

Sh

ukhr

at A

lladu

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Quan

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enh

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d no

n-lin

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scop

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txer

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saci

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Red

mea

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para

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mea

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pola

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sens

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OC

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m H

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an

Bico

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Cub

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Phas

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En

caps

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Char

lotte

Con

n

1700

-171

5Im

pact

of h

ighl

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arge

d io

ns c

reat

ed b

y a

fem

to-

seco

nd X

-ray

pul

se o

n th

e bi

olog

ical

mol

ecul

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ruct

ure

reco

nstru

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exan

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ozlo

v

Sear

chin

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r Tra

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nt

Dark

Mat

ter S

igna

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tom

ic C

lock

Ne

twor

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in R

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Resu

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Prob

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rays

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o an

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na

now

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hn S

cott

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tron

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tom

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ecul

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Ravs

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tam

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Mid

-infra

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mol

ecul

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met

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ultip

lexe

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ensi

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sing

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shap

ed fi

bre

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ie

1715

-173

0W

hich

glu

e to

cho

ose?

A

neut

ron-

scat

terin

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of v

ario

us a

dhes

ive

mat

eria

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ffect

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scat

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Aspe

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of D

ark

Mat

ter

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n Cl

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M

ark

Hert

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An a

ttem

pt fo

r the

ther

mal

tra

nspo

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odel

ling

of

fusi

on p

lasm

as b

ased

on

the

stat

istic

al a

ppro

ach

Mas

ayuk

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a

Ruby

Pay

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cott

Prize

Pre

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atio

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Jacq

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o

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neer

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tow

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Hi

gh-P

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ingl

et-

Fiss

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Amir

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poor

Dar

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Ultra

fast

vis

cosi

ty

mea

sure

men

t in

the

ballis

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optic

al tw

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Mad

sen

Diffu

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ght-

shee

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icro

scop

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pe-f

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calc

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imag

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of n

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M

icha

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aylo

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Repe

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evo

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depe

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in

feat

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nano

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Vino

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-174

5A

liter

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nabl

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col

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achy

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wee

vils

usin

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ngle

dia

mon

d bi

opho

toni

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ysta

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Bodo

Wilt

s


1730

-180

0Br

eak

1800

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ENAR

Y SE

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Octa

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Thea

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1800

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ofes

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aine

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The

beg

inni

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of g

ravit

atio

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ave

astro

nom

yIn

trodu

ced

by S

ean

Salte

r (W

oods

ide)

Co C

hairs

- D

avid

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ir an

d To

m R

idsd

ill-S

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1930

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R Gr

ound

Flo

or T

erra

ce, U

nive

rsity

Clu

b-

incl

udes

pre

sent

atio

n of

Har

rie M

asse

y M

edal

by

Dam

e Ju

lia H

iggi

ns IO

P

Thur

sday

13

Dece

mbe

r 201

8

0730

-180

0Re

gist

ratio

n op

en

Conf

eren

ce F

oyer

, Uni

vers

ity C

lub

0900

-103

0PL

ENAR

Y SE

SSIO

N 5

Octa

gon

Thea

tre

0900

-094

5

0945

-103

0

Prof

Mon

ika

Rits

ch-M

arte

(M

edic

al U

nive

rsity

of I

nnsb

ruck

, Aus

tria)

– B

iom

edic

al O

ptic

s, H

olog

raph

y an

d Op

tical

Tra

ppin

gCh

air:

Halin

a Ru

bins

ztei

n-Du

nlop

Prof

Gar

th Il

lingw

orth

(UC

Sant

a Cr

uz/L

ick

Obse

rvat

ory)

– G

alax

ies

at C

osm

ic D

awn:

Exp

lorin

g th

e Fi

rst B

illion

Yea

rs w

ith th

e Hu

bble

Spa

ce T

eles

cope

Chai

r: Ca

thry

n Tr

ott

1030

-110

0M

orni

ng T

ea

Gro

und

Floo

r Ter

race

, Uni

vers

ity C

lub

1100

-123

0CO

NCUR

RENT

SES

SION

10

Sess

ion:

10A

- AIP

Ast

ron

and

Astr

o +

Fo

cus

Next

-gen

Ast

ro w

ith

new

obs

erva

torie

s

10B

- AIP

Nuc

lear

& P

artic

le

Phys

ics

10C

- AIP

CM

M

10D

- AIP

ATM

OP

10E

- AIP

QUI

CC

10F

- AIP

QUI

CC

10G

- A

OS/A

COFT

10

H - A

IP B

ioph

ysic

s &

Soft

Mat

ter P

hysi

cs

Topi

c:M

icro

wav

e,Te

rahe

rtz, O

ptic

al

and

X-Ra

y sp

ectro

scop

yEx

otic

ato

mic

sys

tem

s an

d ap

plic

atio

nsSp

ins

and

qubi

tsQu

antu

m in

form

atio

n pr

oces

sing

, ion

trap

sSt

ruct

ured

ligh

t and

mat

eria

l in

tera

ctio

ns

Chai

r:Li

ster

Sta

vele

y-Sm

ithM

icha

el P

aul

Step

hen

Thur

gate

Ni

ck R

obin

sJi

angf

eng

DuXi

nhua

Pen

gJo

hn H

arve

yEv

elyn

e De

plaz

es

Room

:Ph

ysic

s Bu

ildin

g Cl

ews

Lect

ure

Thea

tre

[2.4

3]

Phys

ics

Build

ing

Ross

Lec

ture

The

atre

[G.4

1]Ar

ts B

uild

ing

Room

8 [1

.60]

Arts

Bui

ldin

g Ro

om 9

[1.6

1]Ar

ts B

uild

ing

Fox

Lect

ure

Thea

tre

[G.5

9]Ar

ts B

uild

ing

Aust

in L

ectu

re T

heat

re

[1.5

9]

Univ

ersi

ty C

lub

Audi

toriu

mAr

ts B

uild

ing

Room

5 [G

.61]

1100

-113

0Sc

ienc

e hi

ghlig

hts

from

the

ASKA

P ra

dio

tele

scop

e

Elai

ne S

adle

r

Trac

king

the

emer

genc

e of

‘s

impl

e’ c

olle

ctive

nuc

lear

ex

cita

tions

in n

ucle

i. Ho

w d

o th

ey a

rise

from

the

unde

rlyin

g co

mpl

ex n

ucle

onic

mot

ion?

An

drew

Stu

chbe

ry

Tera

hertz

Fre

quen

cy

Phen

omen

a in

Con

dens

ed

Mat

ter a

nd M

ater

ials

Phy

sics

Ro

ger L

ewis

Drop

let c

ryst

al g

roun

d st

ates

of

a d

ipol

ar B

ose

gas

Blai

r Bla

kie

Supe

rradi

ance

and

th

erm

aliza

tion

in h

ybrid

qu

antu

m s

yste

ms

Ka

e Ne

mot

o

Diffe

rent

ial e

volu

tion

for i

on-

trap

gate

des

ign

Barr

y Sa

nder

s

Stru

ctur

ed li

ght f

or n

ano-

and

m

icro

man

ipul

atio

n Ha

lina

Rubi

nszt

ein-

Dunl

op

Phys

ics

of c

ell a

dhes

ion:

The

ro

le o

f the

mem

bran

e in

the

prot

ein

reco

gniti

on p

roce

ss

Henn

ing

Stum

pfAn

a-Su

ncan

a Sm

ith

1130

-114

5Th

e Ph

ase

II M

urch

ison

W

idefi

eld

Arra

y: C

urre

nt

Stat

us a

nd F

utur

e Pl

ans

Mel

anie

Joh

nsto

n-Ho

llitt

Phys

ics

of th

e no

n-He

rmiti

an

free

para

ferm

ion

Z(N)

spi

n ch

ain

Mur

ray

Batc

helo

r

Adva

nced

liqu

id c

ryst

allin

e m

ater

ials

for l

aser

ap

plic

atio

ns c

hara

cter

ised

w

ith h

igh-

Tran

smis

sion

of

light

(T>

97.5

%) a

nd v

ery

low

Refl

ectio

n (R

<0.

7%)

at V

ISib

le, N

ear,

Shor

t and

M

ediu

m In

fraRe

d re

gion

s Zb

igni

ew R

aszw

eski

Nove

l Cor

rela

tions

nea

r an

Orbi

tal F

eshb

ach

Reso

nanc

e Em

ma

Laird

Mic

row

ave

mixi

ng b

y a

stro

ngly

drive

n qu

antu

m d

otM

ark

Hogg

Trap

ped

ion

fast

gat

es s

cale

fa

vour

ably

in m

icro

trap

arra

ys in

the

pres

ence

of

mic

rom

otio

n Jo

e Ho

pe

Tow

ards

sta

biliz

atio

n of

an

optic

ally

levit

ated

mac

rosc

opic

m

irror

Ji

nyon

g M

a

Sphe

rical

tilin

gs w

ith A

BC s

tar

polym

ers

- a

thre

e co

lore

d Th

omso

n pr

oble

m?

Tobi

as H

ain

1145

-120

0On

the

orig

in o

f asy

mm

etric

fis

sion

Ce

dric

Sim

enel

Ultra

sens

itive

Mic

row

ave

Spec

trosc

opy

of S

pin

Ense

mbl

es in

Mul

ti-M

ode

Diel

ectri

c Cr

ysta

l Res

onat

ors

at 2

0 m

K M

d Ak

hter

Hos

ain

Fini

te-t

empe

ratu

re d

ynam

ics

of s

hock

wav

es in

an

ultra

-co

ld F

erm

i gas

Ri

a Jo

seph

Nucl

ear E

lect

ric R

eson

ance

of

the

7/2

spin

of a

sin

gle

123S

b io

n Vi

ncen

t Mou

rik

Ex-v

acuu

m p

hase

Fre

snel

le

nses

for T

rapp

ed Io

n Qu

antu

m In

form

atio

n Pr

oces

sing

Er

ik S

tree

d

Robu

st th

erm

o-op

tic

stab

ilisat

ion

of o

ptic

al s

prin

gs

Paul

Alti

n

Self-

asse

mbl

y of

cub

ic p

hase

s in

pea

r-sh

aped

nan

opar

ticle

sy

stem

s Ph

ilipp

Sch

önhö

fer


Sess

ion:

10A

- AIP

Ast

ron

and

Astr

o +

Fo

cus

Next

-gen

Ast

ro w

ith

new

obs

erva

torie

s

10B

- AIP

Nuc

lear

& P

artic

le

Phys

ics

10C

- AIP

CM

M

10D

- AIP

ATM

OP

10E

- AIP

QUI

CC

10F

- AIP

QUI

CC

10G

- A

OS/A

COFT

10

H - A

IP B

ioph

ysic

s &

Soft

Mat

ter P

hysi

cs

1200

-121

5Th

e SK

A-Lo

w A

pertu

re A

rray

Verifi

catio

n Sy

stem

: res

ults

an

d pl

ans

Rand

all W

ayth

Deep

Neu

ral N

etw

orks

for

anal

ysis

of r

are

B-de

cays

at

Belle

and

Bel

le II

M

artin

Sev

ior

X-Ra

y Sp

ectro

met

ry b

y M

icro

calo

rimet

ry -

Mul

ti De

tect

or S

yste

m w

ith re

al

time

data

ana

lysis

St

ephe

n Th

urga

te

A fin

ite te

mpe

ratu

re m

odel

of

the

early

uni

vers

e Ki

ng N

g

Imag

ing

valle

y in

terfe

renc

e to

ta

ckle

exc

hang

e va

riatio

ns fo

r do

nors

in s

ilicon

Be

noit

Vois

in

High

Per

form

ance

Ram

an

Mem

ory

with

Spa

tio-t

empo

ral

Reve

rsal

Ka

run

Paul

Ther

mod

ynam

ic m

icro

scop

ic

mac

hine

Sh

u Zh

ang

Equi

libriu

m re

ason

ing

for

activ

e pa

rticl

es -

wha

t doe

s it

real

ly m

ean?

Re

né W

ittm

ann

1215

-123

0JW

ST S

tatu

s: In

sigh

ts in

to th

e Ch

alle

nges

of C

onst

ruct

ing

the

mos

t Com

plex

Spa

ce

Tele

scop

e Ev

er

Gart

h Ill

ingw

orth

Acce

lera

tor M

ass

Spec

trom

etry

: the

Sta

te o

f its

Ar

t with

a 1

5MV

Acce

lera

tor

Keith

Fifi

eld

Inte

ract

ion

of B

esse

l-bea

m-

stru

ctur

ed u

ltras

hort

lase

r pu

lses

with

tran

spar

ent m

edia

Lu

dovi

c Ra

pp

Gouy

pha

se in

terfe

rom

eter

an

d its

app

licat

ions

M

umta

Hen

a M

usta

ry

Rota

tion-

sym

met

ric e

ncod

ings

of

a q

ubit

into

an

osci

llato

r Be

n Ba

ragi

ola

Sing

le-p

hoto

n no

n-re

cipr

ocal

tra

nspo

rt co

ntro

lled

by a

si

ngle

ato

m

Keyu

Xia

High

-spe

ed th

ree-

dim

ensi

onal

di

rect

opt

ical

forc

e m

easu

rem

ent

Tim

o Ni

emin

en

Soft

inte

ract

ions

in th

e Lo

rent

z m

odel

: ano

mal

ous

trans

port

in

crow

ded

med

ia

Char

lotte

Pet

erse

n

1230

-133

0Lu

nch

Gro

und

Floo

r Ter

race

- U

nive

rsity

Clu

b

1245

-131

5De

cada

l Pla

n To

wn

Hall

Mee

ting

Phy

sics

Bui

ldin

g, R

oom

215

1245

-144

5AO

S Co

unci

l Mee

ting

Sem

inar

Roo

m 1

, Uni

vers

ity C

lub

1330

-150

0CO

NCUR

RENT

SES

SION

11

Sess

ion:

11A

- A

IP A

stro

n an

d As

tro

+ F

ocus

Nex

t-ge

n As

tro

with

ne

w o

bser

vato

ries

11B

- AIP

Nuc

lear

& P

artic

le

Phys

ics

11C

- AIP

CM

M11

D - A

IP A

TMOP

11E

- AIP

QUI

CC

11F

- AIP

QUI

CC

11G

- AOS

/ACO

FT

11H

- AIP

Com

plex

Sys

tem

s &

Com

puta

tiona

l Phy

sics

Topi

c:Sp

ace

Scie

nce

and

Defe

cts

in

diam

ond

Quam

tum

mea

sure

men

tSp

in q

ubits

and

app

licat

ions

Spin

and

Top

olog

ical

qua

ntum

co

mpu

ting

Nano

stru

ctur

es, p

lasm

onic

s an

d m

etas

urfa

ces

Chai

r:Cl

audi

a La

gos

Andr

ew S

tuch

bery

Alas

tair

Stac

ey

Jesp

er L

evin

sen

Geof

f Pry

deM

ile G

uRo

bert

McL

augh

linTo

bias

Hai

n

Room

:Ph

ysic

s Bu

ildin

g Cl

ews

Lect

ure

Thea

tre [2

.43]

Phys

ics

Build

ing

Ross

Lec

ture

The

atre

[G.4

1]Ar

ts B

uild

ing

Room

8 [1

.60]

Arts

Bui

ldin

g Ro

om 9

[1.6

1]Ar

ts B

uild

ing

Fox

Lect

ure

Thea

tre

[G.5

9]Ar

ts B

uild

ing

Aust

in L

ectu

re T

heat

re [1

.59]

Univ

ersi

ty C

lub

Audi

toriu

mAr

ts B

uild

ing

Room

5 [G

.61]

1330

-134

5Gl

obal

21-

cm s

igna

l fro

m

Cosm

ic D

awn

and

the

Epoc

h of

Rei

oniza

tion

Ravi

Sub

rahm

anya

n

Sim

ple

(but

not

too

sim

ple)

de

scrip

tions

of p

artic

le d

ark

mat

ter

Nico

le B

ell

Spac

e ph

ysic

s re

sear

ch

proj

ects

at R

MIT

Phy

sics

Ga

il Ile

s

Quan

tum

con

trol o

f phy

sica

lly

rota

ting

qubi

ts

Andy

Mar

tin

Quan

tum

Con

trol o

f Spi

ns in

So

lids

Jian

gfen

g Du

Zero

- to

ultr

alow

-fiel

d nu

clea

r m

agne

tic re

sona

nce

and

its

appl

icat

ions

Xi

nhua

Pen

g

Plas

mon

ic a

ppro

ache

s to

op

tical

info

rmat

ion

proc

essi

ng

Ann

Robe

rts

Gras

sman

n Ph

ase

Spac

e Th

eory

for F

erm

ions

Br

yan

Dalto

n

1345

-140

0Br

ain-

like

colle

ctive

dyn

amic

s in

a n

euro

mor

phic

nan

owire

sw

itch

netw

ork

Zden

ka K

unci

c

1400

-141

5Fo

reca

stin

g an

d in

terp

retin

g ob

serv

atio

ns o

f the

firs

t ga

laxie

s an

d th

e Ep

och

of

Reio

nisa

tion

Sim

on M

utch

Dete

rmin

atio

n of

pre

cisi

on

fusi

on c

ross

sec

tions

with

a

supe

rcon

duct

ing

sole

noid

al

sepa

rato

r La

uren

Bez

zina

Mag

netic

circ

ular

dic

hroi

sm

spec

trosc

opy

of th

e ni

troge

n-va

canc

y ce

ntre

in d

iam

ond

Mic

hael

Bar

son

Corre

late

d el

ectro

n-io

n pa

irs

as a

sou

rce

of h

eral

ded

ions

An

drew

McC

ullo

ch

Silic

on-v

acan

cy c

entre

s in

na

nodi

amon

ds fo

r eng

inee

red

quan

tum

app

licat

ions

La

chla

n Ro

gers

Engi

neer

ing

long

itudi

nal

coup

ling

in M

ajor

ana

qubi

t sy

stem

s Th

omas

Sm

ith

III-V

sem

icon

duct

or re

sona

tors

on

insu

lato

r for

nan

osca

le

nonl

inea

r opt

ics

Moh

sen

Rahm

ani

Com

bini

ng C

ompu

tatio

nal

Phys

ics

and

Evol

utio

nary

Al

gorit

hms

to C

reat

e Ne

w

Tailo

red

for P

urpo

se G

ranu

lar

Mat

eria

ls

Gary

Del

aney

1415

-143

0M

easu

ring

the

evol

utio

n of

th

e ea

rly U

nive

rse

with

radi

o ob

serv

atio

ns o

f the

Moo

n Be

njam

in M

cKin

ley

A Le

ptoq

uark

Mod

el to

Add

ress

Fl

avou

r Ano

mal

ies

and

Gene

rate

Ra

diat

ive N

eutri

no M

ass

Inne

s Bi

gara

n

Prim

al s

urfa

ce d

efec

ts o

f di

amon

d: s

urfa

ce n

oise

so

urce

s

Alas

tair

Stac

ey

Spin

ning

spi

ns: e

xplo

ring

rota

tiona

l phy

sics

with

qu

antu

m s

enso

rs

Alex

ande

r Woo

d

Spin

cha

rge

sepa

ratio

n w

ith

quan

tum

crit

ical

ity

Xiw

en G

uan

Topo

logi

cal Q

uant

um

Com

puta

tion

with

Non

-Abe

lian

Vorte

x An

yons

Ta

pio

Sim

ula

Mac

hine

Lea

rnin

g fo

r Vis

cous

Dr

ag o

f Par

ticle

s in

a F

luid

La

chla

n Gi

bson

1430

-144

5As

troph

ysic

al A

nd S

pace

W

eath

er S

tudi

es o

f In

terp

lane

tary

Sci

ntilla

tion

with

th

e M

urch

ison

Wid

efiel

d Ar

ray

John

Mor

gan

Prec

isio

n m

ultip

le C

oulo

mb

exci

tatio

n in

Cd-

111

with

GR

ETIN

A Be

n Co

ombe

s

Incr

ease

d d

ensi

ty o

f flu

ores

cent

def

ects

in

diam

ond

by h

igh t

empe

ratu

re

elec

tron

beam

irra

diat

ion

Phili

pp R

eine

ck

Ther

mal

ly-ro

bust

spi

n co

rrela

tions

bet

wee

n tw

o at

oms

Stua

rt S

zige

ti

Disc

over

y an

d en

gine

erin

g of

opt

ical

ly-ad

dres

sabl

e sp

in-d

efec

ts in

dia

mon

d an

d he

xago

nal b

oron

nitr

ide

Mar

cus

Dohe

rty

Eval

uatio

n of

Thr

esho

ld fo

r To

polo

gica

l Cod

es u

nder

bi

ased

noi

se

Wei

-Wei

Zha

ng

Reve

rsib

le C

ontro

l of t

he

Imag

e Co

ntra

st v

ia T

herm

ally

Tuna

ble

Met

asur

face

s

Khos

ro Z

ange

neh

Kam

ali

Unive

rsal

hid

den

orde

r in

am

orph

ous

cellu

lar

geom

etrie

s Ge

rd S

chro

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Conference Foyer: .................................................................... Registration DeskBanquet Hall: ............................................................................. Exhibition and cateringBanquet Hall/Banquet Hall Foyer/Lower Colonnade: ...... PostersGround Floor Terrace: .............................................................. Welcome Reception/Dinner/Thursday cateringSeminar Room 1: ...................................................................... Diversity and Equity Group in Australian Physics Workshop

Ground Level FloorplanUniversity Club of Western Australia


Upper Level FloorplanUniversity Club of Western Australia

Auditorium: .....................ANFF workshop (Sunday only) and Concurrent sessions (Mon-Thurs)Club Restaurant: ...........Physics Education Group High Tea


University of Western Australia Map

University Club of Western Australia: ....ANFF workshop, exhibition, posters, catering, social functions, concurrent sessions, workshopsArts Building: ...............................................Concurrent sessionsPhysics Building: ........................................Concurrent sessionOctagon Theatre: ........................................Plenary sessions and Public LectureAccommodation: ........................................Trinity, St Catherine’s, St George’s


UNIVERSITY PARTNERS

Curtin University’s Department of Physics and Astronomy is rapidly growing in student numbers and high-impact research outputs. Following the award of the low-frequency component of the Square Kilometre Array to Western Australia, the department has organised its undergraduate teaching and research around the areas of astrophysics, applied physics, materials science and theoretical physics. Curtin University is ranked in the top 2% of universities globally with around 56,000 students in campuses in Perth, Kalgoorlie, Dubai, Malaysia, Mauritius and Singapore.

W: curtin.edu.au

The University of Western Australia (UWA) is one of Australia’s leading universities and has an international reputation for excellence in teaching, learning and research. Established in 1911 UWA is one of the oldest universities in Australia. UWA is a World Top 100 university, ranked first in WA.

Amongst the University’s distinguished alumni are two Nobel Prize winners in medicine and a Fields Medallist in mathematics. UWA’s leafy campus on the banks of the Swan River is host to over 23,000 undergraduate, postgraduate and research students across four Faculties, Engineering and Mathematical Sciences, Science, Health and Medical Sciences and Arts, Business, Law and Education.

W: uwa.edu.au

WELCOME RECEPTION

At the CNBP we use the power of light to measure, seeking to understand the complex molecular processes that underpin the living body, as well as other dynamic biological systems. Our approaches and technologies encompass Discovery—of chemical, nanomaterial and fibre based light responsive tools—that Sense and that can also Image. Bringing these three core capability areas together, we are driving the development of innovative new molecular sensing tools that have broad application across the biosciences, medical, agriculture, food and manufacturing sectors. We have research focused nodes at the University of Adelaide, Macquarie University, RMIT University and Griffith University.

W: cnbp.org.au

SUNDOWNER POSTER SESSION

The Optical Society (OSA) is a leading professional organization that provides quality research, inspired interactions and dedicated resources for its extensive global network of optics and photonics experts. Learn more at osa.org.

W: osa.org

sponsors and exhibitors

The Australian Institute of Physics Congress 2018 Committee gratefully acknowledge our sponsors and exhibitors.


NOBEL PRIZE LECTURE

Sponsoring Professor Rainer Weiss

Woodside is Australia’s largest independent oil and gas company with a global portfolio, recognised for world-class capabilities – as an explorer, a developer, a producer and a supplier of energy. Woodside’s technology strategy has been recently updated to ensure a continuing focus on conventional oil and gas technologies and data-driven breakthroughs, while also prioritising carbon management and the development of new energy sources.

W: woodside.com.au

PLENARY LECTURE

Sponsoring Professor Philippa Browning

ANSTO leverages great science to deliver big outcomes. We partner with scientists and engineers and apply new technologies to provide real-world benefits.

Our work improves human health, saves lives, builds our industries and protects the environment.

ANSTO is the home of Australia’s most significant landmark and national infrastructure for research. Thousands of scientists from industry and academia benefit from gaining access to state-of-the-art instruments every year.

To contact ANSTO you can call the main switchboard on +61 2 9717 3111

P: 02 9717 3111W: ansto.gov.auA (Sydney): New Illawarra Road, Lucas

Heights NSW 2234A (Melbourne): 800 Blackburn Road, Clayton

VIC 3168

The Australian Research Council Centre of Excellence for Quantum Computation and Communication Technology (CQC2T) is working to create a universal quantum computing ecosystem. CQC2T undertakes world-class research in silicon and optical quantum computing, quantum communication, quantum interconnects and other quantum technologies. The centre is headquartered at UNSW and comprises more than 200 researchers from seven of Australia’s top research institutions, forming one of the largest combined and focused efforts in quantum computation and communication in the world.

E: [email protected]: cqc2t.orgTwitter: @QuantumC2TLinkedIn: cqc2t

KEYNOTE SPEAKER TRAVEL

The ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav) is using the historic first detections of gravitational waves to understand extreme physics and warped spacetime, and to test the limits of Einstein’s theory of General Relativity.

OzGrav brings together disciplines spanning advanced instrumentation to big data and astronomy. Through our cutting edge research, OzGrav aims to inspire young people into careers in science and technology, and educate the public about the Universe. It is a partnership between Swinburne University, ANU, Monash, University of Melbourne, University of Adelaide and UWA.

Contact: Professor Matthew Bailes, Swinburne University

W: ozgrav.org


INDUSTRY DAY

The Institute of Physics is a leading scientific membership society working to advance physics for the benefit of all. Alongside professional support for its members, it engages with policymakers and the public to increase awareness and understanding of the value that physics holds for all of us.

Its subsidiary company, IOP Publishing, is a world leader in scientific communications, publishing journals, ebooks, magazines and websites globally.

W: iop.org A: 37 Caledonian Road, London N1 9BU

SESSION SPONSOR

Established under the National Collaborative Research Infrastructure Strategy, the Australian National Fabrication Facility (ANFF) provides academia and industry with access to more than 500 state-of-the-art micro/nanofabrication facilities spread across 21 Australian institutions.

For more than a decade ANFF has been enabling research through a mixture of training, expert support and direct access.

From proving principles to producing prototypes, the network is helping to bring about new generations of medical devices, materials, electronics, photonics, and more.

P: 03 9902 9619E: [email protected]: anff.org.auA: 151 Wellington Road, Clayton VIC 3168

AOS PARTNER DAY

SPIE, the international society for optics and photonics, was founded in 1955 to advance light-based technologies. With over 18,000 individual and 650 corporate members from more than 160 countries, the not-for-profit society serves the entire global photonics community. SPIE enables innovation—from fundamental research to product development—through conferences, exhibitions, publications, professional development, and industry advocacy. In 2018, SPIE provided $4 million in support of education and outreach programs.

W: spie.org

DE-GAP Brunch

The Australian Research Council Centre of Excellence for Engineered Quantum Systems (EQUS) unites leading researchers from five Australian universities in building quantum machines that harness the full spectrum of quantum physics. We will solve the most challenging research problems at the interface of basic quantum physics and engineering, and work with partners in industry to translate these research discoveries into practical applications and devices. Our capacity building programs will train a new generation of scientists in cutting-edge fundamental research, innovation, and entrepreneurialism, and ultimately have a major impact on Australia’s high-tech economy.

W: equs.org


PHYSICS EDUCATION GROUP (PEG) HIGH TEA

IOP Publishing is a society-owned scientific publisher, providing impact, recognition and value for the scientific community.

Wholly owned by the UK Institute of Physics (iop.org), we work closely with researchers, academics, and partners worldwide to produce academic journals, ebooks, conference series, and digital products, covering the latest and best research in the physical sciences and beyond.

Any profit IOP Publishing makes goes directly to the Institute to support its activities.

Visit ioppublishing.org for more information

Contact: Fiona Walker, Global Exhibitions & Conference Manager

P: +44 (0)1179 301281W: ioppublishing.org

EDUCATION GRANT

The Nanotechnology field is one of the fastest growing areas of research and technology. The Australian Nanotechnology Network (ANN), is dedicated to substantially enhancing Australia’s research outcomes in this important field by promoting effective collaborations, exposing researchers to alternative and complementary approaches from other fields, encouraging forums for postgraduate students and early career researchers, increasing nanotechnology infrastructure, enhancing awareness of existing infrastructure, and promoting industry and international links.

The ANN will achieve these goals through its dedication to bringing together all the various groups working in the field of Nanotechnology and related areas within Australia.

The International Conference on Nanoscience and Nanotechnology is the major forum designed to achieve these goals.

W: ausnano.net

NAME BADGE/LANYARDS

IPAS is one of six world-leading research institutes at the University of Adelaide. The mission of IPAS is to use the power of light to make the world healthier, wealthier and safer. We are doing this by building unique sensors which harness the powerful properties of light.

W: adelaide.edu.au/ipas

CONTRIBUTING SPONSOR

Institute of Advanced Studies

The Institute of Advanced Studies brings researchers from all over the world to The University of Western Australia, with the aim of further enhancing UWA’s global research profile.

W: ias.uwa.edu.au

PEOPLE’S CHOICE POSTER AWARD

The IEEE Western Australia Section caters for the needs of all IEEE members in Western Australia. The Section has an ongoing programme of technical events.

W: ewh.ieee.org/r10/w_australia/


CONFERENCE SUPPORTED BY

Perth Convention Bureau (PCB) is Western Australia’s official convention bureau that assists in driving business tourism into the state.

PCB works collaboratively with our Western Australian industry members to ensure every event is an outstanding success. We offer funding and support to association conferences, corporate and incentive meetings. Our services are complimentary and are designed to assist you with areas such as funding, bidding, planning and marketing your conference, corporate meeting or incentive group.

Experience a truly extraordinary conference in Perth - a modern, vibrant, world class city that is breathtakingly beautiful, surrounded by natural wonders and set on the banks of the stunning Swan River.

W: pcb.com.au

EXHIBITION BOOTHS

The AIP is the leading professional body working to promote the role of physics in research, education, industry and the community both in Australia and Internationally. Physics provides the basis for much of our current understanding of the world as well as underpinning many established and emerging technologies and is important to Australia’s cultural and economic development. Come and discuss membership options and the benefits of becoming an AIP member.

W: aip.org.au

Coherent Scientific specialises in the supply and support of scientific lasers, spectroscopy systems, microscopes and related equipment. We are the local distributor for highly reputable companies such as Andor, Aerotech, Bruker, Coherent Inc, LakeShore, Nikon, Quantel and TMC.

We have supported our customers for almost 30 years with our experienced sales and service personnel located throughout Australia and New Zealand.

W: coherent.com.au

Ezzi Vision’s core business is the supply of vacuum, glove box and thin film coating equipment to universities, research & scientific institutes and industrial companies.”With over 30 years of combined vacuum technology experience, Ezzi Vision can provide you with products, service, training, and customer support like no other supplier”. Housing over more than 18 different dealerships and 1600 varied products through our facilities in Melbourne and Sydney, we also offer our customers service contracts covering both normal and preventative maintenance.

Ezzi Vision is truly a one stop shop for complete vacuum solutions.

P: 1800 463 994E: [email protected]: ezzivision.com.au


IOP Publishing is a society-owned scientific publisher, providing impact, recognition and value for the scientific community.

Wholly owned by the UK Institute of Physics (iop.org), we work closely with researchers, academics, and partners worldwide to produce academic journals, ebooks, conference series, and digital products, covering the latest and best research in the physical sciences and beyond.

Any profit IOP Publishing makes goes directly to the Institute to support its activities.

Visit ioppublishing.org for more information

Contact: Fiona Walker, Global Exhibitions & Conference Manager

P: +44 (0)1179 301281W: ioppublishing.org

If your research involves perovskite or organic semiconductor energy level determination, visit KP Technology’s booth. We offer an integrated measurement system for EF, EV, HOMO and Eg determination. Our innovative, cost-effective equipment features in over 700 publications for perovskites, solar cells, diamond, metal-oxides, organic semiconductors, OLEDs, nanowires etc. 2018 sees the launch of our new data analysis package, KP WIZE, an ideal accompaniment to our award-winning ambient-pressure photoemission spectroscopy (APS) systems.

E: [email protected]: kelvinprobe.com

Lastek is an exclusive distributor for leading manufacturers in the photonics marketplace such as Toptica, Light Conversion, Gentec-EO, Thorlabs and many others; and have installed our equipment at leading institutions across Australia and New Zealand. Our portfolio covers a vast range of applications, from spectroscopy to atom optics, microscopy to electrochemistry, advanced manufacturing and more.

P: 08 8443 8668E: [email protected]: lastek.com.au

NewSpec specialises in the sales and service of high-end scientific equipment to the scientific research, aerospace & defence, and life science markets throughout Australia and New Zealand. NewSpec is the distributor for leading international manufacturers including;

• Newport Corporation• Spectra-Physics Lasers• Princeton Instruments• Hitachi High-Technologies Electron

Microscopy• NKT Photonics• Avantes• Kentek• Zygo Metrology

P: 08 8463 1967E: [email protected]: newspec.com.au


Quark Photonics is a leading supplier of scientific instrumentation serving the Australian and New Zealand scientific research, defence, industrial and life science markets, specialising in spectroscopy and photonics instrumentation.

Contact: Anthony QuinnM: 0419 240 146E: [email protected]: quarkphotonics.com.au

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Warsash Scientific is a leading Australian supplier of scientific instruments and components serving Australian and New Zealand research, defence and industry since 1976.

We specialise in Nano-positioning, Nano-spectroscopy, Lasers & Photonics, MEMS characterisation, Nano-lithography, and Thin Film technologies including

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With more than 200 Nobel Prize winners among the authors of our books and journal articles, it is safe to say that Springer has earned its place among the world’s foremost STM publishers. As an e-first company our editors discover the best authors and help to disseminate their research, while our developers deliver the next big thing in scholarly communications. Our dedicated teams crisscross the globe to get journal articles, books, protocols and other products into the hands of the researchers, librarians and practitioners who need them most.

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POSTER PROGRAM

Poster Session – Monday 10 December5.30pm – 6.30pm

NO PRESENTER POSTER TITLE

AIP - ASTRONOMY AND ASTROPHYSICS

1 James Beattie Queensland University of Technology

Fractal Geometry through the Sonic Scale of the World’s Largest Turbulence Simulations

2 Gurashish Singh Bhatia International Centre for Radio Astronomy Research (ICRAR)

The Central Redundant Array Mega-Tile at the Murchison Radio Astronomy Observatory

3 Charles Gravestock University of Western Australia

The Phase Synchronisation System for the Mid-Frequency Square Kilometre Array Radio Telescope

4 Paul Hancock Curtin University

Space Situational Awareness with the Murchison Widefield Array

AIP - ATOMIC & MOLECULAR PHYSICS

5 Srivatsa Badariprasad University of Melbourne

Instability of Rotationally-Tuned Dipolar Bose-Einstein Condensates

6 Francis Bayocboc University of Queensland

Dynamics of thermalisation of two tunnel-coupled quasicondensates

8 Julian Berengut University of New South Wales

AMBiT: A program for high-precision relativistic atomic structure calculations

9 Dashavir Chetty Griffith University

Strong field excitation of Argon with few-cycle laser pulses

10 Jonathan Dean University of Melbourne

Absolute energy of the K alpha emission spectrum of Scandium

11 Zhi-Tao Deng University of Queensland

Properties of Superfluid Flow Between Reservoirs

12 Bernard Field Monash University

Variational approach for modelling Bose polarons at finite temperature

13 Daniel Flynn University of Melbourne

Muonic hydrogen and the proton radius problem

14 Dmitry Fursa Curtin University

Electron-impact dissociation of molecular hydrogen

16 Guillaume Gauthier University of Queensland

Transport Dynamics of an Atomtronic LRC Circuit

17 Amy Geddes University of New South Wales

Saturated configuration interaction calculations for five-valent Ta and Db

18 Rohan Glover Griffith University

Frustrated tunneling ionization dynamics with CEP locked pulses

19 Kwan Goddard Lee University of Queensland

Non-Symmetric Vortex equilibria in a Boes-Einstein condensate

20 Joshua Guanzon University of Queensland

Simulation of the Jarzynski equality in a finite temperature Bose gas


22 John McFerran University of Western Australia

Comparison of frequency-to-voltage converters for laser frequency stabilisation and cooling of atoms

23 Matt Reeves University of Queensland

Bistability and non-equilibrium condensation in a driven-damped atomic superfluid

24 Oliver Sandberg University of Queensland

Exact Floquet analysis of time-averaged trapping potentials

25 Grace Sawyer Curtin University

Electron collisions with negative ions

26 Matthew van Eck Curtin University

Cross Sections and Spin Asymmetries for Electron Collisions with Lead Atoms

27 Raymon Watson EQUS University of Western Australia

Optical dipole trapping of ytterbium for an optical lattice clock

28 Daniel Wells University of Melbourne

A phase space perspective on high harmonic generation using Wigner quasiprobability distributions

AIP - BIOPHYSICS & SOFT MATTER PHYSICS

29 Declan Armstrong University of Queensland

Three Dimensional Manipulation and Force Measurement of Microorganisms

30 Azin Azadi Murdoch University

3D printed mechanical meta-materials and bone scaffolds: non-linear elastic behaviour in a “severed” Diamond network.

31 Itia Favre-Bulle University of Queensland

High speed multiple particle tracking for biological applications

32 Jan Gluschke University of New South Wales

Monolithic complementary nafion-gated nanowire circuits with kHz response for bioelectronics applications

33 René Wittmann Heinrich-Heine-Universität Düsseldorf

Density functional theory for two-dimensional hard rods

AIP - COMPLEX SYSTEMS & COMPUTATIONAL PHYSICS

34 Snezhana I. Abarzhi University of Western Australia

Effect of noise on Rayleigh-Taylor mixing with time-dependent acceleration


Stability of an accelerated hydrodynamic discontinuity

36 Ryan Kidd University of Queensland

Phase space methods for nonlinear quantum dynamics in atomic BECs



AIP - CONDENSED MATTER & MATERIAL

37 Alireza Aghajamali Curtin University

Xenon Release upon Thermal Annealing of Nanodiamonds: A Molecular Dynamics Study

38 Tomi Baikie Cambridge University

Singlet Fission Luminescent Solar Concentrators

39 Nicholas Collins University of Melbourne

Towards deterministic implantation of colour centres in diamond

40 Daniel Creedon University of Melbourne

Irradiation induced modification of superconductivity in boron doped diamond

41 Martin Cyster RMIT University

Simulation of low pressure oxidation in Josephson junction fabrication

42 Guochu Deng Australian Nuclear Science & Technology Organization

The Cold-Neutron Triple-Axis Spectrometer SIKA at OPAL

43 Masaaki Doi Tohoku Gaukin University

Magneto-optical Keer Effect of D022-Mn3Ga/Cr/L10-MnGa Trilayered Circler Dots

44 Ruhao Fang University of Sydney

Strain-engineered Ultrahigh Mobility in Phosphorene for Terahertz Frequency Transistors

45 Fabio Isa CSIRO Manufacturing

Nano-diamonds on group-IV semiconductor substrates for quantum optics

46 Mark Johnson University of New South Wales

Electrical control of a single spin-7/2 123Sb donor in 28Si

47 Akib Karim RMIT University

Ab-initio photoluminescence spectrum of NV−centres in small nanodiamonds

48 Mykhailo Klymenko RMIT University

Multi-electron states of phosphorus dopants in silicon nano-structures

49 Mikhail Kostylev University of Western Australia

Effects of hydrogen on the ferromagnetic resonance of Ni80Fe20/Y/Pd multilayer films

50 Ross Leon University of New South Wales

Electrically driven spin qubits with micromagnet in Silicon-MOS quantum dots

51 Hironari Okada Tohoku Gakuin University

Martensitic phase transition under high pressure in Heusler alloy Pd2Mn1+xSn1-x

52 William Pappas ARC Centre of Excellence in Exciton Science

Spatial variation and correlation of spin and magnetoluminescence in organic light-emitting diodes

53 Alexandr Sadovnikov Saratov State University

Brillouin light scattering study of strain-controlled Yttrium Iron Garnet stripes

54 Sergey Samarin University of Western Australia

Spin-orbit interaction on surfaces by spin-polarized (e,2e) spectroscopy

55 Thomas Schefer University of Western Australia

Effect of Hydrogen on the FMR linewidth of thick Co/Pd bilayer systems

56 Toshiyuki Shima Tohoku Gakuin University

Effect of pseudo-diffusion layers on the magnetic properties for artificial Nd-Fe-B grid patterns


57 Irene Suarez-Martinez Curtin University

Graphitization studies using an Atomic Absorption Spectrometer as an ultra-high temperature oven

58 Stuart Watt University of Western Australia

Impact of hydrogen gas on the inverse Spin Hall effect in Pd-Co bi-layer films

AIP - EDUCATION FOR PHYSICS & RELATED DISCIPLINES

59 Rahul Kumar Choudhary University of Western Australia

An analysis of high school students’ attitudes and understanding of Einsteinian physics using short and long interventions

60 Anthony Greaves Swinburne University

An electromagnetic and circuit theory concept inventory of undergraduate engineering students

61 Lorna Jarrett University of Wollongong

Public understanding of key scientific concepts underlying climate change, and suggested learning and teaching strategies to overcome misconceptions

62 Magdalena Kersting University of Oslo & University of Western Australia

How History and Philosophy of Science Can Inform Teaching and Learning of General Relativity in Upper Secondary School

63 Guillermo Munoz Matutano Macquarie University

Educational Toolbox for Photon Correlation Principles and Fundamentals in Quantum Optics

64 Jules Rankin University of Sydney

The Life of a Syllabus: Almost 20 years of HSC Physics.

65 Geoff Swan Edith Cowan University

Short courses for teachers

66 Graham Wild RMIT University

A Matlab based multiple choice marking system graded students’ work, email them a copy of their quiz with computer generated feedback, and provided question analytics to inform intervention and revision.

AIP - GEOPHYSICS, SOLAR, TERRESTRIAL & SPACE PHYSICS

67 Brett Carter RMIT University

The Effect of Plasma Density Variations on the Generalised Rayleigh Taylor Instability in the Equatorial Ionosphere

AIP - GRAVITATIONAL WAVES & RELATIVITY

68 Sebastian Murk Macquarie University

Properties of stress-energy tensor and metric close to the Schwarzschild radius

69 Michael Page University of Western Australia

Enhanced detection of high frequency gravitational waves using unstable optomechanical filters with low loss microresonators

AIP - INDUSTRIAL & APPLIED PHYSICS

70 Ludovic Rapp Australian National University

Evaluation of surface processing efficiency with powerful ultrashort pulse lasers for large-scale industrial applications

71 Jingchao Song University of Melbourne

Large area plasmonic colour pixels via Nanoimprint Lithography

72 Matthew van Breugel Macquarie University

Affordable Nano-scale Thermometry with Diamond



AIP - NUCLEAR & PARTICLE PHYSICS

73 David Dossett University of Melbourne

Automating calibration at the Belle II experiment

74 Greg Lane Australian National University

E6 transition in the decay of Fe-53m

75 Brendan McCormick Australian National University

Relative measurements of g(2+) in the stable even-even Ge and Se isotopes

76 Chandrima Sengupta Australian National University

Elastic Scattering and Reaction cross section of 8Li on heavy and medium mass targets

77 Ben Swinton-Bland Australian National University

Systematic Study of Quasifission in 48Ca-Induced Reactions

78 Anton Wallner Australian National University

Limits in Accelerator Mass Spectrometry for Astrophysical and Nuclear Applications

79 Matt Westlake University Of Wollongong

Characterization and investigations in to phonon dynamics of Silver doped Lanthanum Manganite nano particles for hypothermia treatment of cancer cells.

80 Scott Williams University of Melbourne

Networked cosmic muon detectors for outreach and cosmic muon background measurement

AIP - PLASMA PHYSICS


Late-time evolution of Rayleigh-Taylor instability in a domain of a finite size


Effect of noise on Rayleigh-Taylor mixing with space-dependent acceleration

83 Kavya Hemantha Rao Griffith University

Angle resolved X-ray emission spectroscopy of laser produced metal plasmas and alloys

84 Desmond Hill University of Western Australia

Effect of pressure fluctuations on Richtmyer-Meshkov coherent structures

85 Desmond Hill University of Western Australia

Dimensional crossover in Richtmyer-Meshkov unstable flows in the presence of pressure fluctuations

86 Vishnu Mangalath University of Western Australia

Coordinate-free Grad-Shafranov equation on a Riemannian manifold with Killing field

87 David Pfefferlé University of Western Australia

What may the experimental and numerical data tell us on properties of Rayleigh-Taylor interfacial mixing?

88 David Pfefferlé University of Western Australia

Non-planar elasticae as optimal curves for the magnetic axis of stellarators

AIP - QUANTUM INFORMATION, CONCEPTS & COHERENCE

89 Estelle Asmodelle ARC Centre for Quantum Computation Communication Technology - University of Queensland

Relativistic Bohmian Trajectories


90 Leonardo Assis Morais University of Queensland

Transition edge sensor: photon-number resolving detectors

91 Travis Baker Griffith University

Beyond the Conventional Limit to the Coherence of a Laser

92 Ben Baragiola Centre for Quantum Computing & Communication Technology

Quantum trajectories for the joint state of a system and field

93 Philip Blocher Aarhus University - Department of Physics & Astronomy

Temporally non-local effects in optical detection

94 Kok-Wei Bong Griffith University

Strong unitary and overlap uncertainty relations: theory and experiment

95 Shakib Daryanoosh Macquarie University

Quantum master equations for entangled qubit environments

96 Marcus Doherty Australian National University

Optimisation of diamond quantum processors

97 Tim Evans University of Sydney

Methods in Matrix Product Operator Tomography

98 Florian Frank Institute of Quantum Optics, Ulm University

Closed-loop optimization of single spin control in room-temperature solids

99 Jemy Geordy EQUS & Macquarie University

Bayesian estimation of blinking in nano-diamond color centres

100 Kaumudibikash Goswami University of Queensland

Extracting information from depolarising channels using indefinite causal order

101 Glen Harris University of Queensland

Stable Levitation of Superfluid Helium; Optomechanics with Droplets

102 Sean Hodgman Australian National University

Bogoliubov-Cherenkov Radiation, Machine Learning and Quantum Depletion Experiments with Helium Bose-Einstein Condensates

103 Lewis Howard University of Queensland

Optimal Spatial Metrology

104 Michael Kewming University of Queensland

Ignorance of the whole does not imply ignorance of the parts: Qudit Random Access Codes in spatial modes of light

105 Ruvi Lecamwasam Australian National University

Analysis and feedback-control of a levitating mirror

106 Anthony Leung Australian National University

Storing single photons using gradient echo memory

107 Lucas Mensen RMIT University

Predicting successful error correction in a measurement-based quantum computation with continuous-variable cluster states

108 Gary Mooney University of Melbourne

Gate synthesis using higher orders of the Clifford hierarchy

109 Felix Pollock Monash University

Long-time dynamics from short-time tomography data for driven open quantum processes



110 Nicholas Pritchard University of Western Australia

Cluster-Based Simulation of the Quantum Approximate Optimisation Algorithm

111 Sarath Raman Nair EQUS & Macquarie Unversity

Towards room-temperature lasing with NV centres in open fibre cavities

112 Sarath Raman Nair EQUS & Macquarie Unversity

On the theory of diamond Raman lasers with colour centres in the crystal

113 Rostyslav Savytskyy CQC2T, School of EE&T, University of New South Wales

Tuning the flip-flop qubit of a 31P donor in silicon

114 Jordan Scarabel Griffith University

Towards a Quantum Network with Trapped Ions and Waveguides

115 Oliver Stockdale University of Queensland

Modelling expanding vortex clusters in thin film superfluid helium

116 Ming Su University of Queensland

Asymmetric Quantum Interference Observed Using Photon-number-resolving Detectors

117 Run Yan Teh Swinburne University of Technology

Creation, storage and retrieval of an optomechanical cat

118 Sam Tonetto University of Melbourne

Sampling Boltzmann Distributions with Quantum Annealing

119 Blayney Walshe RMIT University

Fault-tolerant measurement-based quantum computing with impure continuous-variable cluster states

120 Prahlad Warszawski University of Sydney

Optomechanical quantum control of superfluid Helium vortices

121 Keyu Xia Nanjing University

Quantum memory and gates using a Lambda-type quantum emitter coupled to a chiral waveguide

123 Wei-wei Zhang The University Of Sydney

Identification quantum topological phases with neural networks deep learning

AIP - SYNCHROTRON SCIENCE, SCATTERING, MICROSCOPY, IMAGING

124 Dehong Yu Australian Nuclear Science & Technology Organisation

PELICAN – a Multi-Purpose Time-of-Flight Cold Neutron Spectrometer

AOS/ACOFT - BIOPHOTONICS

125 Steven Hinckley Edith Cowan University

Optical coherence tomography modelling incorporating absorption and scattering

126 Jaehwan Kwon Kyungbook University

Micro vibration measurement and surface vibration projection of latex samples using optical Doppler tomography system

127 Oeon Kwon Kyungpook National University

Real-time index regulating technique for direct wavenumber-linearization in spectral domain optical coherence tomography

128 Farah Qazi University of Melbourne

Non-invasive optical imaging of nematode eggs


AOS/ACOFT - NONLINEAR OPTICS

129 Michelle Wang University of Sydney

Short-range surface plasmons for stimulated Brillouin scattering

AOS/ACOFT - OPTICAL DEVICES

130 Raymond Harrison RMIT University

Multi-photon evolution using waveguide adiabatic passage

131 Douglas Little Macquarie University

Quantum-Random Bit Generation using Raman-Laser Pulses in Diamond with Randomly-Oriented Linear Polarisations

132 Ben Sparkes University of Adelaide

High-transmission fibre ring resonator for spectral filtering of master oscillator power amplifiers

AOS/ACOFT - OPTICAL SENSING

133 Steven Hinckley Edith Cowan University

Determining the Displacement of Flexible Membranes using Fibre Bragg Gratings

134 Lu Peng University of Adelaide

Micron-scaled resolution distributed sensing using exposed core fibre

135 Paul Sibley Australian National University

Exploring the performance of Digitally Enhanced Interferometry for Optical Phased Arrays

136 Nonthanan Sitpathom Macquarie University

Shaping of microsphere arrays by plasma treatment for optical sensing

137 Lei Xu University of New South Wales

Hybrid Metasurface Based Polarization Independent Tunable Perfect Absorber and Plasmonic Sensor

AOS/ACOFT - OPTICS, PHOTONICS & LASER PHYSICS

138 Deeksha Beniwal University of Adelaide

Mid-IR fibre lasers for wavefront correction in advanced gravitational wave detectors.

139 Le Gao RMIT University School of Science LAIN Group

Development of optically active solid medium for high-capacity optical data storage

141 Isaac Lenton University of Queensland

OTSLM: A toolbox for production of flexible structured light

142 David McAfee University of Adelaide

An electronically controlled mode-locked thulium all-fibre laser at 1.990µm

143 Jillian Moffatt University Of Adelaide

Energy transfer upconversion parameter for 4I13/2 measured in erbium doped ZBLAN fibre

144 Kerry Mudge Defence Science Technology Group

Scintillation Mitigation Strategies for Asymmetric Free Space Laser Communications

145 Kerry Mudge Defence Science Technology Group

Analysis of Atmospheric Turbulence Effects for Laser Satellite Communications

146 Sascha Schediwy University of Western Australia

Development of an Optical Phased Array to Power Interstellar Travel



147 Mandip Singh Indian Institute of Science Education & Research, Mohali

Three-dimensional imaging of a pattern localized in a phase space

148 Lei Xu University of New South Wales

Highly-efficient normal second-harmonic generation from doubly-resonant AlGaAs nanoantennas

AOS/ACOFT - QUANTUM OPTICS

149 Paul Altin Australian National University

Controlling the squeezing ellipse angle at a 2 micrometer wavelength

150 W Y Sarah Lau University of Queensland

Hectometer Revivals of Quantum Interference

151 Yasmine Sfendla University of Queensland

Proposal for optomechanical single-vortex detection in 2D superfluids

COMMAD - ELECTRON DEVICES & SYSTEMS

152 Weijun Fan Nanyang Technological University

Tensile Strain Effect on Band Structure of Ge and Ge Quantum Well

153 Jeremy Gillbanks University of Western Australia

Reference Electrode-Free pH Sensing at Temperatures above 300 K Using AlGaN/GaN Transistor-Based Chemical Sensors

154 Georgina Carson University of New South Wales

An atomically precise 4-qubit processor using donor spins in silicon

155 Shahbaz Khan University of Western Australia

Response enhancement of a magnetic-film based hydrogen gas sensor using size reduction to microchip dimensions

156 Peter Metaxas University of Western Australia

Spin torque nano-oscillators for electronic, frequency-based, magnetic biosensing

157 Michal Zawierta University of Western Australia

AFM integration with on-chip optical interferometric read-out

COMMAD - OPTOELECTRONICS/PHOTONIC DEVICES & SYSTEMS

158 Minh Nguyen University of Technology Sydney

Nanoassembly of hexagonal boron nitride and gold nanospheres

159 Inseok Yang Australian National University

Single axial n-i-p junction InP nanowires for high performance solar cells

COMMAD - TECHNOLOGIES & THEORIES FOR MICROELECTRONICS, OPTOELECTRONICS & PHOTONICS

160 Yaman Afandi University of Western Australia

Study of Porosity Gradient in Released Porous Silicon Microstructures

161 Gilberto Umana Mebreno Microelectronics Research Group, The University Of Western Australia

Modelling of damping characteristics in silicon-gold bilayer cantilevers


162 Gurpreet Singh Gill University of Western Australia

Modelling and Fabrication of Anti-Stiction Features for Electrostatically Actuated Microsystems

164 Praveen Kumar Revuri University of Western Australia

Si and SiO2 thin films deposited by ICPCVD at low temperature and high deposition rate for MEMS applications

165 Tarun Sanders University of Western Australia

Investigation of a novel method for the fabrication of larger area imaging fibre bundles with greater number of pixels and reduced dead space

166 Pritam Sharma University of Western Australia

Engineering porous silicon thin films to obtain high TCR and low 1/f noise for application in thermal detectors.

167 Jorge Silva Castillo University of Western Australia

Method for optical modelling of non-uniform and non-parallel multi-thin film MEMS optical filters and mirrors

168 Hoe Tan Australian National University

Wafer-scale growth of hexagonal boron nitride on sapphire substrates using metal organic vapour phase epitaxy

269 Jianan Wang University of Western Australia

A Raman spectroscopy study on the surface structural properties of gallium nitride-based materials

FOCUS SESSION - 50 YEARS OF BICONTINUOUS CUBIC PHASES

170 Benjamin Cumming RMIT University

Impact of cubic symmetry on the optical properties of gyroid networks

FOCUS SESSION - OPTICAL & QUANTUM BIO-SENSING

171 Michael Barson Australian National University

Quantum sensing of Neuronal signals

172 Larnii Booth University of Queensland

Quantum limited plasmonic sensing of motor molecule dynamics

173 Pawan Kumar Abbe Center of Photonics, Friedrich-Schiller-Universität Jena

Mid-infrared sensing by induced coherence in a single nonlinear waveguide

174 Cyril Laplane Macquarie University

A new tool for optical manipulation of nano-object based on atomic forces

175 Daniel McCloskey University of Melbourne

Enhancement of Fluorescence from Dense Ensembles of Near-Surface Nitrogen-Vacancy Centres for Biological Sensing

176 Chris Perrella University of Adelaide

Rapid optical measurement of 13CO2 and 12CO2 number density

177 David Simpson University of Melbourne

Diamond based quantum sensing and imaging

178 David Simpson University of Melbourne

Nanoscale intracellular thermometry using diamond quantum probes


presenting authors

AUTHOR AFFILIATION

Abarzhi, Snezhana I. University of Western Australia

Abdurakhmanov, Ilkhom Curtin University

Abrahao, Raphael University of Queensland

Ackley, Kendall Monash University

Ako, Rajour RMIT University

Alladustov, Shukhrat Curtin University

Altin, Paul Australian National University

Aminzadeh, Alaleh La Trobe University

Andersen, Mikkel F University of Otago

Anderson, Malcolm Universiti Brunei Darussalam

Andersson, Gunther Flinders University

Angstmann, Elizabeth University of New South Wales

Antoszewski, Jarek University of Western Australia

Asadpoor Darvish, Amir ARC Centre of Excellence in Exciton Science

Atakaramians, Shakhik University of New South Wales

Babic, Bakir Department of Industry, Innovation and Science

Baikie, Iain KP Technology

Baker, Christopher University of Queensland

Baker, Mark University of Queensland

Balazs, Csaba Monash University

Banerjee, Kaushik Australian National University

Baragiola, Ben ARC Centre for Quantum Computation and Communication Technology

Barberio, Elisabetta University of Melbourne

Barson, Michael Australian National University

Bartlett, Stephen University of Sydney

Bartolo, Tommy RMIT University

Batchelor, Murray Australian National University

Bekker, Christiaan University of Queensland

Beniwal, Deeksha University of Adelaide

AUTHOR AFFILIATION

Bennet, Francis Australian National University

Bennett, James ARC Centre of Excellence for Engineered Quantum Systems

Berengut, Julian University of New South Wales

Berry, Dominic Macquarie University

Bezzina, Lauren Australian National University

Bhansali, Aesha University of Sydney

Bickerton, Oliver University of Sydney

Bigaran, Innes University of Melbourne

Bignall, Hayley CSIRO

Bignell, Lindsey Australian National University

Bioletti, Gabriel Victoria University of Wellington

Bioletti, Gabriel Victoria University of Wellington

Bishop, James University of Technology Sydney

Blackwell, Boyd Australian National University Research School of Physical Sciences and Engineering

Blair, Carl Caltech

Blair, David University of Western Australia

Blake, Samuel University of Sydney

Booth, Jamie RMIT University

Bossilkov, Vladimir University of Western Australia

Botzem, Tim University of New South Wales

Bourhill, Jeremy University of Western Australia

Bradby, Jodie Australian National University

Bradshaw, Mark Australian National University

Bray, Alexander Australian National University

Brennen, Gavin Macquarie University

Broer, Wijnand Nanyang Technological University

AUTHOR AFFILIATION

Budden, Jessica University of New South Wales

Cadusch, Jasper University of Melbourne

Cao, Huy Tuong University of Adelaide

Carrascosa, Eduardo University of Melbourne

Carter, Brett RMIT University

Casacio, Catxere University of Queensland

Castelli, Marina Monash University

Catinella, Barbara University of Western Australia

Causer, Grace University of Wollongong

Cavalcanti, Eric Griffith University

Cha, Jihun University of Queensland

Chantler, Christopher University of Melbourne

Chantler, Christopher University of Melbourne

Chen, Xu University of Western Australia

Cheng, Zhangkai University of Sydney

Chhetri, Rajan International Centre for Radio Astronomy Research

Chiew, Mitchell University of Western Australia

Choudhary, Rahul Kumar

University of Western Australia

Chubb, Chris University of Sydney

Cocks, Danny Australian National University

Colas, David University of Queensland

Cook, Peter Flinders University

Coombes, Ben Australian National University

Copeland, Michael Australian National University

Costa, Fabio University of Queensland

Cumming, Benjamin RMIT University

Cumming, Benjamin RMIT University

Cyster, Martin RMIT University

Dalton, Bryan Swinburne University of Technology


AUTHOR AFFILIATION

Dasgupta, Mahananda Australian National University

Daszuta, Boris University of Otago

Dawes, Judith Macquarie University

De Lacy, Kooper University of Western Australia

De Tomas, Carla Curtin University

Dean, Jonathan University of Melbourne

Dehdashti, Nima University of Western Australia

Delaney, Gary CSIRO

Deng, Guochu Australian Nuclear Science and Technology Organisation

Devitt, Simon University Of Technology, Sydney

Doherty, Marcus Australian National University

Dotera, Tomonari Kindai University

Dowie, Jackson Australian National University

Duong, Ngoc My Hanh University of Technology Sydney

Ebert, Martin University of Western Australia

Ehrig, Sebastian Max Planck Institute of Colloids and Interfaces

Elliman, Robert Australian National University

Elliman, Robert Australian National University

Farrant, David CSIRO

Favre-Bulle, Itia University of Queensland

Favre-Bulle, Itia University of Queensland

Fifield, Keith Australian National University

Firth, Daniel Bioimaging Research and Innovation for Translational Engineering

Fleming, Simon University of Sydney

Fleming, Simon University of Sydney

Flower, Graeme University of Western Australia

Foot, Robert University of Sydney

Galloway, Duncan Monash University

AUTHOR AFFILIATION

Gambell, Adam University of Adelaide

Gardiner, Bruce Murdoch University

Geddes, Amy University of New South Wales

Ghafari, Farzad Griffith University

Giarmatzi, Christina University of Queensland

Gibson, Lachlan University of Queensland

Gluschke, Jan University of New South Wales

Gluschke, Jan University of New South Wales

Golde, Jonas TU Dresden

Gomez, Daniel RMIT University

Gopalakrishnan, Dhaneesh Kumar

Monash University

Gorman, Sam ARC Centre of Excellence for Quantum Computation and Communication Technology

Goryachev, Maxim University of Western Australia

Gozzard, David Australian National University

Greybush, Nicholas U.S. Naval Research Laboratory

Gu, Mile Nanyang Technological University

Guan, Xiwen Chinese Academy of Sciences Wuhan Physics and Mathematics Institute

Gurusamy, Jega Thisan University of Western Australia

Hain, Tobias Murdoch University

Hannaford, Peter Swinburne University of Technology

Haram, Nida Griffith University

Harper, Robin University of Sydney

Harris, Rob University of Queensland

He, Xin (Eric) University of Queensland

Hepburn, Matt Harry Perkins Institute of Medical Research

Herrera Benzaquen, Ivan

Swinburne University of Technology

Hertzberg, Mark Tufts University

AUTHOR AFFILIATION

Higginbottom, Daniel Australian National University

Hill, Desmond University of Western Australia

Hinckley, Steven Edith Cowan University

Hinckley, Steven Edith Cowan University

Hitchman, Sam AgResearch

Hodgman, Sean Australian National University

Hodgman, Sean Australian National University

Hogg, Mark University of New South Wales

Hoinka, Sascha Swinburne University of Technology

Hole, Matthew Australian National University

Hope, Joe Australian National University

Hora, Heinrich University of New South Wales

Hosain, Md Akhter University of Western Australia

Hosseinidehaj, Nedasadat

University of Queensland

Howell, Eric University of Western Australia

Huang, Lujun University of New South Wales

Huang, Wister (Wei) University of New South Wales

Huebner, Moritz Monash University

Huf, Peter Deakin University

Hui, Hui Swinburne University of Technology

Hurley-Walker, Natasha International Centre for Radio Astronomy Research

Illingworth, Garth UC Santa Cruz

Ironside, Charlie Curtin University

Jaberian Hamedan, Vahid

University of Western Australia

Jarrett, Lorna University of Wollongong

Jay, Gareth University of Western Australia

Joseph, Ria Rushin Swinburne University of Technology

Kane, Deb Macquarie University


AUTHOR AFFILIATION

Kane, Deb Macquarie University

Karouta, Fouad Australian National University

Keating, Adrian University of Western Australia

Keith, Daniel ARC Centre for Quantum Computation and Communication Technology

Kersting, Magdalena University of Western Australia

Kheruntsyan, Karen University of Queensland

Kish, Sebastian University of Queensland

Klymenko, Mykhailo RMIT University

Kobakhidze, Archil University of Sydney

Koll, Dominik Australian National University

Korzekwa, Kamil University of Sydney

Kozlov, Alexander University of Melbourne

Kranz, Ludwik ARC Centre for Quantum Computation and Communication Technology

Krasnokutska, Inna RMIT University

Krohn, Jo-Frederik University of Melbourne

Kuncic, Zdenka University of Sydney

Lagos, Claudia University of Western Australia

Laird, Emma Monash University

Lamon, Simone RMIT University

Lane, Greg Australian National University

Langford, Nathan University of Technology Sydney

Laverick, Kiarn Griffith University

Lavin Varela, Sebastian Australian National University

Lazendic-Galloway, Jasmina

Monash University

Lebedev, Petr University of Sydney

Lenton, Isaac University of Queensland

Levinsen, Jesper Monash University

Li, Beibei Institute of Physics Chinese Academy of Sciences

Li, Jiawen University of Adelaide

Li, Jiawen University of Adelaide

AUTHOR AFFILIATION

Li, Xuegang University of Adelaide

Light, Philip University of Adelaide

Light, Philip University of Adelaide

Little, Douglas Macquarie University

Litvinyuk, Igor Griffith University

Liu, Xia-Ji Swinburne University of Technology

Lobino, Mirko Griffith University

Lund, Austin University of Queensland

Lung, Shaun Australian National University

Ma, Jinyong Australian National University

Madsen, Lars University of Queensland

Madzik, Mateusz University of New South Wales

Mahmood, Ibtihal University of Melbourne

Malajczuk, Christopher Curtin University

Malik, Umairia University of New South Wales

Marsh, Samuel University of Western Australia

Mauranyapin, Nicolas University of Queensland

McAllister, Benjamin University of Western Australia

McCamey, Dane University of New South Wales

McCann, Joshua University of Western Australia

McCoey, Julia University of Melbourne

McCulloch, Andrew University of Melbourne

McGloin, David University of Technology Sydney

Mckinley, Benjamin Curtin University

McMahon, Nathan Macquarie University

McManus, David Australian National University

Meadors, Grant Monash University

Melville, Graeme University of New South Wales

Mendelson, Noah University of Technology Sydney

Meng, Chao University of Queensland

Meng, Jiajun University of Melbourne

AUTHOR AFFILIATION

Metaxas, Peter University of Western Australia

Miller-Jones, James International Centre for Radio Astronomy Research

Miroshnichenko, Andrey University of New South Wales

Mitchell, AJ Australian National University

Mitchell, Emma CSIRO

Morgan, John Curtin University

Mourik, Vincent University of New South Wales

Mulkerin, Brendan Swinburne University of Technology

Munoz Matutano, Guillermo

Macquarie University

Mustary, Mumta Hena Griffith University

Mutch, Simon University of Melbourne

Neely, Tyler University of Queensland

Neshev, Dragomir Australian National University

Neshev, Dragomir Australian National University

Ngampruetikorn, Vudtiwat

Northwestern University

Nguyen, Quan Griffith University

Nieminen, Timo University of Queensland

Nieminen, Timo University of Queensland

Nuti, Francesco University of Melbourne

Pan, Wenwu University of Western Australia

Panchenko, Evgeniy University of Melbourne

Pantaleoni, Giacomo RMIT University

Panther, Fiona Helen Australian National University

Parish, Meera Monash University

Paul, Karun Australian National University

Pavetich, Stefan Australian National University

Peace, Daniel Griffith University

Peng, Jingyang RMIT University

Perrella, Chris University of Adelaide

Perunicic, Viktor University of Melbourne


AUTHOR AFFILIATION

Petersen, Charlotte University of Innsbruck

Phan, Hoang-Phuong Griffith University

Piecek, Wiktor Military University of Technology

Pollock, Felix Monash University

Pumarol Crestar, Manny Monash University

Quach, James University of Adelaide

Quinn, Peter University of Western Australia

Quinton, Jamie Flinders University

Quinton, Jamie Flinders University

Rachel, Stephan University of Melbourne

Radhanpura, Krunal CSIRO

Rahmani, Mohsen Australian National University

Raj, Vidur Australian National University

Ralph, Tarquin Australian National University

Rapp, Ludovic Australian National University

Raszewski, Zbigniew Military University of Technology

Reece, Peter University of New South Wales

Regan, Blake University of Technology Sydney

Reichardt, Christian University of Melbourne

Reineck, Philipp RMIT University


Roberts, Benjamin Paris Observatory

Roberts, Benjamin Paris Observatory

Rogers, Lachlan Macquarie University

Rogers, Lachlan Macquarie University

Rule, Kirrily Australian Nuclear Science and Technology Organisation

Rule, Kirrily Australian Nuclear Science and Technology Organisation

Sachkou, Yauhen University of Queensland

Sanders, Yuval Macquarie University

Sanderson, Rowan University of Western Australia

Saranathan, Vinodkumar

Yale NUS College

AUTHOR AFFILIATION

Savytskyi, Mykhailo University of New South Wales

Scarlett, Liam Curtin University

Schediwy, Sascha University of Western Australia

Schediwy, Sascha University of Western Australia

Schmidt, Mikolaj Macquarie University

Schmitt, Simon University of Ulm

Schön, Yannick Karlsruhe Institute of Technology

Schönhöfer, Philipp Murdoch University

Schroeder-Turk, Gerd Murdoch University

Schuyt, Joseph Victoria University of Wellington

Scott, John University of Technology Sydney

Scutti, Federico University of Melbourne

Sevior, Martin University of Melbourne

Seymour, Nicholas International Centre for Radio Astronomy Research

Sharma, Abhishek University of Adelaide

Shi, Zheyu Monash University

Simenel, Cedric Australian National University

Simpson, Edward Australian National University

Simula, Tapio Swinburne University of Technology

Slussarenko, Sergei Griffith University

Smith, Rory Monash University

Smith, Thomas University of Sydney

Solntsev, Alexander University of Technology Sydney

Spagnoli, Dino University of Western Australia

Sparkes, Ben University of Adelaide

Spollard, James Australian National University

Stace, Tom University of Queensland

Stace, Tom University of Queensland

Stacey, Alastair University of Melbourne

Stadnik, Yevgeny Johannes Gutenberg University of Mainz

AUTHOR AFFILIATION

Stavrevski, Daniel ARC Centre of Excellence for Nanoscale BioPhotonics

Streed, Erik Griffith University

Suarez-Martinez, Irene Curtin University

Sullivan, Hugh RMIT University

Sun, Qiang University of Melbourne

Sun, Xiao University of Western Australia

Szigeti, Stuart Australian National University

Tam, Kevin University of Sydney

Taylor, Michael University of Queensland

Taylor, Michael University of Queensland

Tee, Bryan Pi Ern Australian National University

Terno, Daniel Macquarie University

Tetienne, Jean-Philippe University of Melbourne

Thompson, Jayne National University of Singapore

Thomson, Catriona University of Western Australia

Thrane, Eric Monash University

Thurgate, Stephen Murdoch University

Tischler, Nora Griffith University

Titov, Oleg Geoscience Australia

Tobar, Michael University of Western Australia

Tonekaboni, Behnam University of Queensland

Tranter, Aaron Australian National University

Tretiakov, Oleg University of New South Wales

Tripathi, Dhirendra University of Western Australia

Tserkis, Spyros University of Queensland

Twamley, Jason Macquarie University

Twamley, Jason Macquarie University

Uhrig, David Victoria University of Wellington

Ungar, Goran University of Sheffield

Ungaro, Francesca University of Melbourne

Usman, Muhammad University of Melbourne


AUTHOR AFFILIATION

Utamuratov, Ravshanbek

Curtin University

Vaccaro, Joan Griffith University

van Heijningen, Joris University of Western Australia

Varvell, Kevin University of Sydney

Vidal, Xavier Macquarie University

Vogl, Tobias Australian National University

Voisin, Benoit University of New South Wales

Wallner, Anton Australian National University

Wang, Jia Swinburne University of Technology

Wang, Naiyin Australian National University

Warren-Smith, Stephen University of Adelaide

Watkins, Craig Informative Technology Innovations

Wayth, Randall Curtin University

Webb, James University of Melbourne

Webster, Paul University of Sydney

Wegener, Margaret University of Queensland

Wilkinson, Samuel RMIT University

Wilts, Bodo University of Fribourg

Wittmann, René University of Düsseldorf

Wood, Alexander University of Melbourne

Woolley, Matt University of New South Wales

Worboys, Josef RMIT University

Wu, Shengling University of Sydney

Xia, Keyu Nanjing University

Xie, Liushun University of Adelaide

Xu, Lei University of New South Wales

Yang, Inseok Australian National University

Yap, Min Jet Australian National University

Yap, Min Jet Australian National University

Yokoyama, Masayuki National Institute for Fusion Science

Zakaria, Azwa University of Queensland

Zangeneh Kamali, Khosro

Australian National University

AUTHOR AFFILIATION

Zhang, Shu University of Queensland

Zhang, Wei-wei University of Sydney

Zhang, Wen Qi University of South Australia

Zhang, Jue University of Western Australia

Zhao, Chunnong University of Western Australia

Zhao, Jiangbo Leibniz Institute of Photonic Technology

Zhao, Zijun University of Sydney

Zhu, Xingjiang Monash University

Zhu, Xingjiang Monash University

Zych, Magdalena University of Queensland

Abarzhi, Snezhana I. University of Western Australia

Abasahl, Banafsheh Imec

Aharonovich, Igor University of Technology Sydney

Ares, Natalia University of Oxford

Aspelmeyer, Markus

Aspelmeyer, Markus

Bailes, Matthew Swinburne University of Technology

Ballato, John Clemson University

Barberio, Elisabetta University of Melbourne

Bell, Nicole University of Melbourne

Bell, Nicole University of Melbourne

Bertram, John Monash University

Bezak, Eva University of South Australia

Blakie, Blair University of Otago

Bowen, Warwick University of Queensland

Bray, Igor Curtin University

Burde, Jan-Philipp University of Frankfurt

Cairney, Julie University of Sydney

Cense, Barry University of Western Australia

Chen, Zhigang Nankai University

Conn, Charlotte RMIT University

Coppersmith, Susan University of Wisconsin-Madison

Corr, Cormac Australian National University

AUTHOR AFFILIATION

Crozier, Kenneth University of Melbourne

Cushman, Priscilla University of Minnesota

Davis, Matthew University of Queensland

Davis, Tamara University of Queensland

Deplazes, Evelyne Curtin University

Dicker, Jason Department of Education

Du, Jiangfeng University of Science and Technology of China

Ebendorff-Heidepriem, Heike

University of Adelaide

Eilenberger, Falk University of Jena

Ekins-Daukes, Ned University of New South Wales

Fisher, Matthew UC Santa Barbara

Fortier, Tara National Institute of Standards and Technology

Funston, Alison Monash University

Gao, Weibo Nanyang Technological University

Garrett, Richard Australian Nuclear Science and Technology Organisation

Gibson, Brant RMIT University

Giger, Maryellen University of Chicago

Ginges, Jacinda University of Queensland

Grubisic-Cabo, Antonija Monash University

Helmerson, Kristian Monash University

Hinde, Elizabeth University of Melbourne

Hollenberg, Lloyd University of Melbourne

Hyde, Stephen Australian National University

Iles, Gail RMIT University

Jackson, Paul University of Adelaide

Jagadish, Chennupati Australian National University

Johnston-Hollitt, Melanie

Curtin University

Joyce, Hannah University of Cambridge

Ju, Li University of Western Australia

Karakas, Amanda Monash University


AUTHOR AFFILIATION

Kivshar, Yuri Australian National University

Lee, Woei Ming (Steve) Australian National University

Levy, Jeremy University of Pittsburgh

Lewis, Roger University of Wollongong

Li, Wenhui National University of Singapore

Luiten, Andre University of Adelaide

Marquardt, Florian Max Planck Institute for the Science of Light

Martin, Andy University of Melbourne

Mather, Melissa University of Nottingham

McFerran, John University of Western Australia

Miroshnichenko, Andrey University of New South Wales

Moelmer, Klaus Aarhus University

Munro, William NTT Basic Research Laboratories

Murphy, Tony CSIRO

Nakamura, Yasunobu The University of Tokyo

Nemoto, Kae National Institute of Informatics

O'Brien, Jeremy University of Bristol

Paul, Michael The Hebrew University

Peng, Xinhua University of Science and Technology of China

Pfefferlé, David University of Western Australia

Pryde, Geoff Griffith University

Qu, Zhisong Australian National University

Quinn, Peter University of Western Australia

Rahmani, Mohsen Australian National University

Reid, Margaret Swinburne University of Technology


Roberts, Ann University of Melbourne

Robins, Nick Australian National University

Rowell, Gavin University of Adelaide

Rubinsztein-Dunlop, Halina

University of Queensland

Sadler, Elaine University of Sydney

AUTHOR AFFILIATION

Sanders, Barry University of Calgary

Scholten, Sarah University of Adelaide

Shannon, Ryan Swinburne University of Technology

Shi, Yuejiang Seoul National University

Simpson, David University of Melbourne

Simpson, Cather University of Auckland

Singh, Chandralekha University of Pittsburgh

Stuchbery, Andrew Australian National University

Stumpf, Henning University of Erlangen–Nuremberg

Subrahmanyan, Ravi Raman Research Institute

Suchowerska, Natalka University of Sydney

Sushkov, Oleg University of New South Wales

Suter, Melissa Massachusetts General Hospital and Harvard Medical School

Suzuki, Chihiro National Institute for Fusion Science

Terno, Daniel Macquarie University

Thomas, Anthony University of Adelaide

Ting, David NASA Jet Propulsion Laboratory

Urquijo, Phillip University of Melbourne

Villiger, Martin Massachusetts General Hospital

Walmsley, Ian University of Oxford

Walther, Julia TU Dresden

Walus, Konrad University of British Columbia

White, Andrew University of Queensland

Wolf, Peter Paris Observatory

Yang, Shu Zhejiang University

Yuan, Gangcheng University of Melbourne

Zhao, Jie Australian National University

Singh, Chandralekha University of Pittsburgh

Wiescher, Michael University of Notre Dame

Illingworth, Garth UC Santa Cruz

Krauss, Thomas University of York

Odom, Teri Northwestern University

AUTHOR AFFILIATION

Padilla, Willie Duke University

Pan, Jian-Wei University of Science and Technology of China

Ritsch-Marte, Monika Medical University of Innsbruck

Scott, Susan Australian National University

Weiss, Rainer Massachusetts Institute of Technology

Yeomans, Julia University of Oxford

Bell, Thomas University of Queensland

Garraway, Barry University of Sussex

Hall, Liam University of Melbourne

Liu, Junliang University of Western Australia

Neil, Benjamin University of Western Australia

Ng, King Lun Swinburne University of Technology

Savage, Jeremy Curtin University

Wang, Jianan University of Western Australia

Documents

23rd Australian INSTITUTE of Physics Congress · 2. The registration desk will be open for the duration of the congress and will be your main point of contact for all congress related