HEP Research and Technology Division

OverviewDOE/HEP PI Meeting 2018

Glen Crawford

Research and Technology Division Director

Office of High Energy Physics

Office of Science, U.S. Department of Energy

Bottom-line Up Front

Great things are happening!

Important and exciting results across the portfolio

Great future leaders are revealed through Early

Career Awards!

Their ideas are supported by the ECA, with 91 HEP

Awards since 2010

Great new ideas in both science and technology

are emerging from the community, generating

interest and excitement!

We are working on ways to support these new ideas

DOE/HEP PI Meeting 2018 2

FY 2019 Budget Request Highlights

Energy Frontier: Actively engage in successful LHC program and HL-LHC upgrades The High-Luminosity Large Hadron Collider (HL-LHC) ATLAS & CMS detector upgrades (new

MIE starts) and the HL-LHC Accelerator Upgrade Project are together considered one of P5’s highest priority large projects

The U.S. will continue to play a leadership role in LHC discoveries by remaining actively engaged in analysis of world’s highest energy particle collider data

Intensity Frontier: Support establishing U.S.-hosted world-leading neutrino program LBNF/DUNE is P5’s highest priority U.S.-hosted large project, FY19 investments in far-site civil

construction crucial to enable scheduled delivery of contributions from international partners

Support Short-Baseline Neutrino (SBN) program at Fermilab, DUNE prototype R&D efforts at CERN, and continued funding for PIP-II project to upgrade the Fermilab Accelerator Complex

Cosmic Frontier: Advance our understanding of dark matter and dark energy P5 recommended complementary suite of projects to search for dark matter candidates and

study dark energy; request supports full planned profile for LZ, SuperCDMS-SNOLAB, DESI

3DOE/HEP PI Meeting 2018

HEP Research Priorities

Broadly speaking, focus will be (not

necessarily in priority order):

Research activities critical to executing the

upcoming P5 projects;

Supporting initial data taking and analysis from

new experiments coming on-line;

Continued analysis of ongoing experiments highly

recommended to address the P5 science drivers;

and

Supporting young investigators

DOE/HEP PI Meeting 2018 4

DOE HEP Research Priorities: Snapshot

Energy Frontier

Analysis of LHC Run 2 data

Contribute to operational responsibilities and complete “Phase I” upgrades

Scientific support for HL-LHC program

Intensity Frontier

Neutrino Program

Support ProtoDUNE, LBNF/DUNE, and PIP-II

Implement Fermilab Short-Baseline Neutrino Program and Intermediate Neutrino Program

NOvA, T2K/SK, Minerva, MicroBooNE data analysis

Muon Program: Complete Mu2e, take data with Muon g-2

Heavy Flavor Program: take and analyze data with Belle-II

Cosmic Frontier

Dark Matter: Scientific support for G2 experiments (in fabrication)

Dark Energy: DES analysis; scientific support for LSST and DESI (in fabrication)

Continue science planning for CMB-S4

Accelerator R&D

Focus on outcomes and capabilities that will dramatically improve cost effectiveness for mid-term and far-term accelerators

Hosting workshops to develop and implement R&D plan following P5 and GARD panels

Detector R&D

Developing process to identify highest priority R&D activities for current phase of implementing P5

Long-term “high-risk” R&D with potential for wide applicability and/or high-impact

“Blue-Sky” scientific research on innovative technologies not already in contention for implementation in future DOE HEP projects

HEP Theory

Maintain an overall “thriving” program as per P5

DOE/HEP PI Meeting 2018 5

See PM parallel session talks Wed/Thu

FY 2018 Early Career Awards: Univ.

Thomas Faulkner, University of Illinois New perspectives on QFT and gravity from quantum entanglement

Alexie Leauthaud-Harnett, University of California, Santa Cruz Exploiting Synergies Between Lensing and BAO Surveys for Improved

Cosmological Constraints

Themis Mastoridis, California Polytechnic State University Optimal Design of Radio Frequency Algorithms and Models for Next

Generation Accelerators

Benjamin Safdi, University of Michigan Particle Dark Matter Across Scales

Hee-Jong Seo, Ohio University Optimal and robust reconstruction of BAO, redshift-space distortions

and the Alcock-Paczynski effect

David Simmons-Duffin, Caltech Precision Computations in Strongly Coupled Conformal Field Theories

Rachel P. Yohay, Florida State University Probing New Physics with Tau Leptons using the CMS Detector

DOE/HEP PI Meeting 2018 6

FY 2018 Early Career Awards: Labs

Artur Apresyan, FNAL Exploring the Lifetime Frontier with New Detectors and New Searches

Daniel Bowring, FNAL Microwave Single-Photon Sensors for Dark Matter Searches and

Precision Neutrino Measurements

Daniel A. Dwyer, LBNL Improving Neutrino Detection in DUNE with Pixel Sensors

Michael Kagan, SLAC Exploring the Higgs Sector at the Energy Frontier with Bottom Quarks,

Machine Learning, and the Upgraded ATLAS Pixel Detector

Aritoki Suzuki, LBNL Development of high throughput techniques for SC microfabrication,

assembly and deployment for future high energy physics experiments

Kazuhiro Terao, SLAC GPU/FPGA Accelerated Deep Learning Technique Development for

Discovering Physics in Liquid Argon Time Projection Chambers

Javier Tiffenberg, FNAL Towards table-top neutrino detectors: A 10 kg Skipper-CCD

experiment

7

HEP Program Highlights

DOE/HEP PI Meeting 2018 8

Energy Frontier: LHC, ATLAS, and CMS

U.S. ATLAS represents ~19% of the international ATLAS Collaboration 41 universities, 4 national labs (Argonne,

Brookhaven, Lawrence Berkeley, SLAC)

Brookhaven is host lab for U.S. ATLAS

U.S. CMS represents ~29% of the international CMS Collaboration 53 universities, 1 national lab

Fermilab is host lab for U.S. CMS

States hosting members of the U.S. LHC experimental program

The Large Hadron Collider at CERN is the centerpiece of the U.S. Energy Frontier program

Large Hadron Collider Tunnel ATLAS Detector CMS Detector

DOE/HEP PI Meeting 2018 9

HL-LHC Accelerator Upgrades:Enabling U.S. Science Participation

10

DOE contribution:10 cold mass (Nb3Sn)

assemblies • 4 each for

ATLAS & CMS interaction regions

• 2 spares

DOE contribution:Hollow e-Lens Components (under discussion)

DOE contribution:20 Crab Cavities (16 + 4 spares)or: 10 Crab cavities & Hollow e-Lens Components

See M Procario talk (next)

EF Highlight: ttH Production

April 2018 results from ATLAS and CMS on Higgs production in association with a top quark pair

ATLAS combined result observes 4.2σsignificance (3.8σexpected)

Phys. Rev. D 97, 072003

CMS combined result observes 5.2σsignificance (4.2σexpected)

Accepted for Phys. Rev. Lett. [arXiv:1804.02610]

DOE/HEP PI Meeting 2018 11

IEEE Milestone for Tevatron Technology

On Nov. 13, the Institute of Electrical and Electronics Engineers (IEEE) recognized the technological innovations driven by the Tevatron with a prestigious IEEE Milestone Award for the development of the accelerator’s superconducting magnets During construction, 95% percent of the world's niobium-titanium

production went into the Tevatron's 774 superconducting magnets

DOE/HEP PI Meeting 2018 12

“The first large-scale use of superconducting magnets enabled the construction of the Tevatron. By 1985, the Tevatron achieved energy above 1 Tera electron-volt (TeV) in proton-antiproton collisions, making it the most powerful particle collider in the world until 2009. The Tevatron construction established the superconducting wire manufacturing infrastructure that made applications such as Magnetic Resonance Imaging (MRI) viable.”

Future Colliders

DOE coordinating with international community towards development of the next collider program U.S. looks forward to a decision this year by Japan to host the ILC as an international project

Global strategy for circular collider awaits 2020 European Strategy Update for Particle Physics

Interest from HEP community to pursue R&D studies for future collider options Circular collider: DOE efforts focused on high-field magnet technology to enable higher energy

ILC: DOE efforts focused on cost reduction R&D, e.g., nitrogen treatment in SRF cavities has potential for up to 10% cost reductions in 3-5 years, up to 15% in 5-10 years

Near-term priorities aim to support the LHC program including HL-LHC upgrades

High-Q0

(e.g. LCLS-II)

High-Q0; High-Eacc

(e.g. ILC)

SRF cavity:

Nitrogen Treatment R&D

DOE/HEP PI Meeting 2018 13

Intensity Frontier Program

Intensity Frontier experiments address the P5 Science Drivers through intense beams and sensitive detectors

Exploring the unknown through precision measurements: Muon g-2, Muon-to-Electron Conversion Experiment

(Mu2e), Belle II, K0TO

Identify the new physics of dark matter: Heavy Photon Search

Pursuing the physics associated with neutrino mass: NOvA, Daya Bay, MINERvA, Super-K, T2K ongoing

Ramping up Fermilab Short-Baseline Neutrino Program (MicroBooNE, SBND, ICARUS)

Preparing to host world-leading neutrino program with the Long-Baseline Neutrino Facility and Deep Underground Neutrino Experiment (LBNF/DUNE)

Muon g-2

NOvA

Belle II

DOE/HEP PI Meeting 2018 14

Collaboration News

André Rubbia

Phone Call

May 29, 2015

Long-Baseline Neutrino Facility and Deep Underground Neutrino Experiment

IllinoisSouthDakota Long-Baseline Neutrino Facility

IllinoisSouthDakota Long-Baseline Neutrino Facility

P5 recommended Long-Baseline Neutrino Facility (LBNF) as the centerpiece of a U.S.-hosted world-leading neutrino program LBNF will produce the world’s most intense neutrino

beam, send it 800 miles through the earth to DUNE

Strong support within the U.S. Government and many interested potential global partners

International DUNE collaboration includes: Over 1,100 collaborators from 176 institutions, 31 countries

Proton Improvement Plan II (PIP-II) will provide increased proton beam intensity (>1 MW) for LBNF

DOE/HEP PI Meeting 2018 15

Proton Improvement Plan II (PIP-II)

The P5 report recommended that PIP-II proceed immediately in order to provide increased proton beam intensity (of > 1 megawatt) for LBNF Replace the existing 50 year old linear accelerator with a higher power; one

powered by superconducting radiofrequency cavities

Supports longer-term physics research goals by providing increased beam power and high reliability for future experiments at Fermilab, including LBNF/DUNE

Old Fermilab Linac enclosure

New Fermilab Linac enclosure

DOE/HEP PI Meeting 2018 16

See M Procario talk (next)

IF Highlight: COHERENT Observes CEvNS

COHERENT experiment uses the world’s smallest neutrino detector to search for coherent elastic neutrino-nucleus scattering (CEνNS) 14.6-kg CsI[Na] scintillator operating at Oak Ridge National

Laboratory’s Spallation Neutron Source (SNS)

43 years after the first theoretical prediction, COHERENT observed CEvNS at a 6.7σ confidence level “Observation of coherent elastic neutrino-nucleus scattering”

published in Science, August 3, 2017

Characteristic signatures in energy and time, predicted by the Standard Model for this process, are observed in high signal-to-background conditions

DOE/HEP PI Meeting 2018 17

IF Highlight: First Collisions at Belle II

Belle II collaboration includes over 750 researchers from 25 countries and regions Includes a dozen U.S. Universities and Laboratories

U.S. Belle II project delivered key components of imaging Time-Of-Propagation (iTOP) and Klong-Muon (KLM) detector upgrade Received DOE Project Management Achievement

Award for delivering components ahead of schedule and under budget

Belle II aims to collect 50x the data of Belle over 10 years, using the 40x luminosity improvement of SuperKEKB

April 26: First collisions at SuperKEKB, after successfully storing electron and then positron beams in March 2018

DOE/HEP PI Meeting 2018 18

IF Highlight: SBN Far Detector Installation

ICARUS cold vessels now installed at Fermilab! Completed trans-Atlantic trip in July 2017

First cold vessel installed August 9, 2018

Second cold vessel installed August 14, 2018

Planning for data-taking in 2019

DOE/HEP PI Meeting 2018 19

Cosmic Frontier Program I

Cosmic Frontier experiments address the P5 science drivers using naturally occurring cosmic phenomena

In addition to NSF and NASA partnerships, most experiments and projects have international partners or contributions and some also have private contributions

Study dark energy’s role in the accelerating expansion of the universe through staged suite of complementary surveys Enables precision measurements that differentiate between

cosmological constant, modification to gravity, or new fields

Fast, wide area imaging surveys scan large volumes and catch dynamic events like supernovae: Dark Energy Survey (DES) operating, Large Synoptic Survey Telescope (LSST) 3-billion pixel camera in fabrication

Deep, high accuracy spectroscopic surveys study dim, more distant objects: eBOSS operating, Dark Energy Spectroscopic Instrument (DESI) in fabrication

Study inflation in the early universe using its imprint on the cosmic microwave background (CMB) South Pole Telescope 3G is operating, planning for P5-

recommended next-generation CMB Stage 4 experiment underway

AAAC Conceptual Design Team (CDT) developed strawman design (2017), Lab tech. development and pre-Project Design Group (pPDG) studies ongoing

DOE/HEP PI Meeting 2018 20

Cosmic Frontier Program II

Staged suite of dark matter direct detection experiments use multiple technologies to search for WIMP, Axion particles First-generation experiments produced world’s most sensitive

searches

P5-recommended 2nd generation experiments are advancing

ADMX-G2 axion search is operating; LZ and SuperCDMS-SNOLAB WIMP search projects in fabrication

Planning for small project(s) to address new priority science areas to search for dark matter

Pursue the physics associated with neutrino mass Dark Energy and CMB experiments also place unique constraints on

the sum of neutrino masses

Explore the unknown through cosmic- and gamma-ray experiments Perform indirect searches for dark matter and antimatter

Study fundamental physics properties such as breakdown of Lorentz invariance & high energy acceleration mechanisms

Space-based Fermi/GLAST & AMS and ground-based HAWC are currently operating

DOE/HEP PI Meeting 2018 21

Y1 galaxy clustering & weak lensing

CF Highlight: DES Y1 Results

DES studies Dark Energy via survey of 300 million galaxies, 3,000 supernovae with 570-megapixel Dark Energy Camera on Blanco telescope in Chile Planned 5 year ops. began Aug. 2013; extended through Dec. ‘18

Cosmology results from DES Year 1 data Aug. 2017: Galaxy clustering & weak lensing; competitive with Planck

Dec. 2017: Baryon Acoustic Oscillation (BAO) to z=1

Jan. 2018: Data Release 1; first 3 yrs. of survey data

Over 150 papers: most distant supernova, new Milky Way dwarf satellites to constrain dark matter, & more…

DOE/HEP PI Meeting 2018 22

DES Y1 produced largest map of dark matter in the Universe

Y1 BAO results

CF Highlight: ADMX-G2

Axion Dark-Matter eXperiment Generation 2 at U. Washington Uses a strong magnetic field and resonant cavity to convert dark matter

axions into detectable microwave photons

Selected as one of three G2 dark matter experiments following P5

Currently stepping through range 0.5 to 2 GHz (~ 2 to 8 micro-eV)

Dec. 2017 review of operations status (now led by Fermilab)

Results: May 2017: ADMX first experiment to reach Dine-Fischler-Srednicki-

Zhitnitsky (DFSZ) sensitivity limit for any axion mass range!

DOE/HEP PI Meeting 2018 23

Scientific AmericanJanuary 2018

Enabling Discovery though Advanced Technology R&D

Recent results:

Low-Loss Superconducting Radio-Frequency (SRF) Cavities using new processes developed by Fermilab Linac Coherent Light Source II (LCLS-II), under construction by Basic Energy

Sciences (BES), will be first beneficiary

Advances in laser-driven and beam-driven plasma wakefieldaccelerators Could produce high-gradient accelerators for future machines

Record current in high-temperature superconductors Could enable magnetic field levels that double existing particle collision

energies

DOE/HEP PI Meeting 2018 24

Advanced Technology R&D supports and advances research at all three experimental Frontiers

Fosters cutting-edge research in the physics of particle beams, accelerator R&D, and particle detection

Three broad categories: Near- to mid-term directed R&D for facilities/technologies in support of current DOE projects

Mid-term, facility-inspired R&D focused on concepts or technologies to demonstrate feasibility

Long-term, proposal-driven research on the fundamental science to enable breakthroughs in size, cost, beam intensity, beam energy, and control

Theoretical and Computational Physics

Provides the mathematical, phenomenological, and computational framework to understand and extend our knowledge of the dynamics of particles and forces, and the nature of space and time

Theoretical research essential for proper interpretation and understanding of the experimental research activities in other HEP subprograms

Advanced computing tools necessary for designing, operating, and interpreting experiments and scientific simulations that enable experimental discovery research

QIS: First HEP QIS call for proposals complete, see next slide for details

Implementing the P5 strategy requires advancing computing infrastructure to handle the exponentially increasing data and computing needs Partnerships with Advanced Scientific Computing Research (ASCR)

are an important part of addressing HEP computing needs

HEP aims to optimally leverage DOE resources in developing future computing solutions to meet mission needs

Cross-cutting efforts aim to prepare for future of computing, especially Exascale facilities

DOE/HEP PI Meeting 2018 25

FY 2018 QIS FOA & Lab Announcement

Quantum Information Science Enabled Discovery (QuantISED) for High Energy Physics

Closed April 16, 2018 HEP received an enthusiastic response!

Objective: Forge new routes to scientific discovery along HEP mission and P5 science drivers, invoking interdisciplinary advances in the convergent field of QIS, and intersection with expertise, techniques, technology developed in HEP community

Topics:

A: High Energy Physics and QIS Research

B: Quantum Computing for HEP on current or future quantum computing systems

Track 1: Pioneering Pilots (open to Topics A or B)

Work scope: Novel concepts, test problems, design studies (TRL 1)

Award: $100k - $500k over 1-2 years

Track 2: HEP-QIS Consortia (Open to Topic A only)

Work scope: Address P5, small experiments, early research on tools (TRL 1-2)

Award: FOA 500k – $2M (FOA) or $1M - $4M (LAB) over 2-3 years

Public announcement of selected HEP QIS proposals in Sept!

DOE/HEP PI Meeting 2018 26

See L Chatterjee talk (Wed PM)

Accelerator Stewardship

Mission: Support fundamental accelerator science and technology development of relevance to many fields and to disseminate accelerator knowledge and training to the broad community of accelerator users and providers.

Improve access to national lab accelerator facilities Make resources and facilities, such as Brookhaven National

Laboratory’s Accelerator Test Facility II (ATF-II), available for industrial and for other U.S. government agency users and developers of accelerators and related technology

Develop innovative solutions to critical problems outside of the DOE Office of Science More performant, lower cost accelerators for medicine

1000x speedup of laser-based science tools

Accelerator tech. for Energy & Environmental applications

Broaden and strengthen the community Bringing accelerator scientists, application scientists, and

industrialists together to address high-impact challenges

DOE/HEP PI Meeting 2018 27

See E Colby talk Thu AM

P5 Implementation Planning

In addition to executing P5 recommended

projects, DOE/HEP has developed processes

to examine the research portfolio and guide

implementation

Balance small and large investments

Establish R&D milestones and goals

Examine new ideas

GARD Workshops

HEP Portfolio Review

Basic Research Needs Workshops

DOE/HEP PI Meeting 2018 28

Adv. Tech. R&D: Research Roadmaps

Following the release of the HEPAP Accelerator R&D Subpanel Report in April 2015, the General Accelerator R&D (GARD) Program has engaged its research community to address the Subpanel recommendations to develop research roadmaps for these thrust areas: Superconducting High Field Magnets

Produced the U.S. Magnet Development Program Plan

Advanced Accelerator Concepts

Laser-driven plasma wakefield acceleration (LWFA)

Particle-beam-driven plasma wakefield acceleration (PWFA)

Dielectric wakefield acceleration (DWFA)

Radiofreqency Acceleration Technology

Superconducting RF

Normal Conducting RF

RF Sources

Community-developed roadmaps include: Pressing challenges to be addressed to move the field forward

Prioritized milestones aligned to the most compelling science

DOE/HEP PI Meeting 2018 29

Roadmaps Summary

Technology R&D Roadmaps are already having an impact in the HEP program Laboratory and University communities are aligning their efforts to meet the roadmap goals

Technology R&D Subprogram is using the roadmaps to guide program implementation

Progress and alignment will be assessed in lab accelerator R&D comparative review this summer

Roadmaps have also identified opportunities for possible applications of HEP Technology R&D to other program offices in the Office of Science Discussions are underway for opportunities where investments would have broad benefits

DOE/HEP PI Meeting 2018 30

HEP Portfolio Review

Portfolio Review assessed 13 currently operating HEP-supported experiments and prioritized their impact on P5 science drivers: 4 Tiers, from absolutely essential to “less effective”

HEP will prioritize ongoing support for top-Tier(s)

U.S. contributions to LHC experiments also examined, with generally high praise and a few comments

No DOE action will be taken in response to Portfolio Review recommendations without discussing with domestic and international partners Specific DOE guidance to experiments in response to

portfolio review recommendations will be sent in September 2018

DOE/HEP PI Meeting 2018 31

Basic Research Needs Workshops (BRNs)

SC’s Office of Basic Energy Sciences initiated this approach with the Basic Research Needs to Assure a Secure Energy Future workshop in October 2002. This resulted in a comprehensive, 420-page report that identified 37 Proposed Research Directions.

Numerous (~20) subsequent topically-focused BRNs have helped to define directions and make the case for major new efforts such as Energy Frontier Research Centers and Innovation Hubs

While there are some variations and there has been some evolution, many BRNs have involved:

Production of a Technology Perspectives Factual Document prior to the workshop

Definition of a set of Priority Research Directions that address the technology R&D challenges

Definition of a set of Science Grand Challenges that, if solved, might result in transformational changes

DOE/HEP PI Meeting 2018 32

BRN Process and Structure

Targeted topics defined by, and workshop charge issued by, SC program office

Attendance is limited and by invitation

Participants will have considerable work to do before, during, and after the meeting

Workshop Chair and Co-Chairs develop agenda and select panel leads (with program office input)

Typical structure: Opening plenary sessions, panel breakout sessions that develop priority research directions, closing plenary session, and extended writing session – draft report completed before departure!

Prompt output: final report released typically 60-90 days after the workshop

DOE/HEP PI Meeting 2018 33

BRN Impacts

BRN reports are expected to serve as reference documents with a long shelf life, and to be readily accessible

Post-workshop outreach activities often include communication of the results to the broader community by co-chairs and the SC program, and briefings by federal staff to other interested federal parties (within and beyond DOE)

BRNs may, individually or collectively, serve as the basis for subsequent funding opportunities. Examples:

An FY2007 FOA on Basic Research for Advanced Nuclear Energy Systems was based directly on the corresponding BRN, stating specifically that “The workshop report is a current source of information and summarizes the interests of BES.”

The original FY2009 solicitation for the Energy Frontier Research Centers (up to $100M/yr total) centered on the 11 BRNs that SC-BES had held to date

DOE/HEP PI Meeting 2018 34

HEP Basic Research Needs Workshops I

BRN workshop on New Opportunities for Dark Matter March 2017 community workshop held to determine scientifically

compelling areas to search and possible concepts for new experiments or studies

White Paper: https://arxiv.org/abs/1707.04591

Considering P5 recommendations and the current landscape, HEP will hold a BRN on Dark Matter in October 2018 to:

Identify priority science opportunities for new directions and areas of phase space that will provide significant science return and advancement.

Of these:

Which technology needs for which concepts for new small projects could be ready to go in the near term?

Which would be best carried out using DOE infrastructure and capabilities?

Co-Chairs have been identified and are starting to organize

Detector R&D is being considered for a future BRN workshop in 2019

DOE/HEP PI Meeting 2018 35

HEP Basic Research Needs Workshops II

BRN workshop on Compact Accelerators for Security and Medicine is in the planning stages for the coming year Focused on near-term applications

(3-5 years) of compact accelerator technologies to security and medical applications

Will identify high impact applications, technical gaps requiring basic R&D, and the primary barriers to technology adoption

Will identify required application-side R&D

Engage the other stakeholder federal agencies and provide a roadmap for near-term compact accelerator R&D, with particular attention given to technology transfer to industry

Will be by invitation only

DOE/HEP PI Meeting 2018 36

Image credit: LLNL

Image credit: 10.3390/ijms15069878

Summary

Great things are happening!

Important and exciting results across the portfolio

Great future leaders are revealed through Early

Career Awards!

Their ideas are supported by the ECA, with 91 HEP

Awards since 2010

Great new ideas in both science and technology

are emerging from the community, generating

interest and excitement!

We are working on ways to support these new ideas

DOE/HEP PI Meeting 2018 37

The Science Drivers of Particle Physics

The U.S. long-term strategy report identified five intertwined science drivers, compelling lines of inquiry that show great promise for discovery:

Use the Higgs boson as a new tool for discovery

Pursue the physics associated with neutrino mass

Identify the new physics of dark matter

Understand cosmic acceleration: dark energy and inflation

Explore the unknown: new particles, interactions, and physical principles

*2013

*2015

*2011

* Since 2011, three of the five science drivers havebeen lines of inquiry recognized with Nobel Prizes

DOE/HEP PI Meeting 2018 39

Enabling the Next Discovery

P5 identified 5 Science Drivers to address the scientific motivation in particle physics

Research Frontiers are useful categorization of experimental techniques and serve as the basis of the budget process

Research Frontiers arecomplementary No one Frontier addresses

all science drivers

Each Frontier provides adifferent approach toaddress science driver

Enables cross-checkingscientific results

DOE/HEP PI Meeting 2018 40

CMS HL-LHC Upgrade

DOE and NSF coordinating U.S. contributions with CERN and international partners on CMS Scope of the U.S. deliverables leverages expertise by U.S. scientists

3.8

*

*

Significant U.S. contributions

NSF

DOE NSF

DOE

DOE

NSF

= Significant

U.S. contributions

NSF

DOE

DOE/HEP PI Meeting 2018 41

ATLAS HL-LHC Upgrade

Similarly, U.S. ATLAS is defining the scope of its contributions to HL-LHC by leveraging interests and experience of U.S. groups, coordinating with international ATLAS

* Large forward rapidities, as described in the 2015 ATLAS HL-LHC scoping document (for the reference 275 MCHF CORE total cost scenario)

DOE Scope: Barrel Inner Tracker

(pixel & strip detector)

LAr Calorimeter front-end analog chip development

DAQ hardware (data flow elements)

NSF Scope: ‘Triggering’ at high

luminosities

Readout electronics for LAr, Tile, Muons

DOE/HEP PI Meeting 2018 42

LBNF/DUNE in South Dakota

Large-scale cryogenic vessel will house state-of-the-art neutrino detector one mile underground

215 ft.

61 ft.

Sanford Underground Research FacilityLead, South Dakota (U.S.)

55 ft.

Personfor Scale

4 cryostats at 10-ktons each

DOE/HEP PI Meeting 2018 43

Advancing Technology Towards LBNF/DUNE

Fermilab Short-Baseline Neutrino Program Resolve experimental anomalies in measured -spectrum, including search for sterile neutrino

Demonstrate the detector technology for DUNE

The largest liquid argon neutrino detector in the world, ICARUS was transported from Europe to Fermilab First major item of equipment to ship for the

international neutrino program

Far Detector – ICARUS (760-ton LAr)to be installed – Fall 2017

MiniBooNE

MicroBooNE(existing)

170-ton LAr

Fermilab Short-Baseline Neutrino Complex

DOE/HEP PI Meeting 2018 44

Program Advice and Coordination Formal advice (Federal Advisory Committee Act)

High Energy Physics Advisory Panel (HEPAP)

Jointly serves DOE and National Science Foundation (NSF)

2014: P5 long-term strategy report

2015: Accelerator R&D Subpanel report

Astronomy and Astrophysics Advisory Committee (AAAC)

Advises DOE, NSF, and NASA on selected issues of mutual interest within the fields of astronomy and astrophysics (e.g. CMB-S4 Conceptual Design Team)

Community input National Academies of Science: Astronomy and Astrophysics Decadal

Survey (New Worlds, New Horizons)

DOE Workshop reports, including Quantum Sensors, Accelerator R&D Roadmaps, Technology Connections, Basic Research Needs, etc.

International coordination CERN Council (LHC)

Governs CERN by defining its strategic programs, setting and following up its annual goals, and approving its budget

International Neutrino Council (LBNF/PIP-II)

International consulting body for DOE that facilitates high-level global coordination across the LBNF/PIP-II enterprise

Resources Review Board (DUNE)

Facilitates Fermilab’s coordination of resource-related matters for DUNE

DOE/HEP PI Meeting 2018 45

HEP FY 2019 Budget Request

Details

DOE/HEP PI Meeting 2018 46

FY 2019 President’s Budget Request

2019 President’s Budget Request for HEP is overlay of Administration, SC, P5 priorities SC: interagency partnerships, national laboratories, accelerator R&D, QIS

P5: preserve vision, modify execution

FY19 Budget Request reduces near-term science for P5-guided investments in mid- and long-term program “Building for Discovery” by supporting highest priority P5 projects to enable future program

Research support advances P5 science drivers and world-leading, long-term R&D in Advanced Technology, Accelerator Stewardship, and Quantum Information Science

Operations support enables world-class research at HEP User Facilities

The Administration and Congress support the overall P5 strategy FY19 House Mark for HEP: $1,004,510,000 ; FY19 Senate Mark for HEP: $1,010,000,000

DOE/HEP PI Meeting 2018 47

HEP Funding Category ($ in K)

FY 2017 Actual

FY 2018 Enacted

FY 2019 Request

FY 2019 vs.

FY 2018

Research 344,043 369,565 280,130 -89,435

Facilities/Operations 258,696 260,535 211,020 -49,515

Projects 222,261 277,900 278,850 +950

Total 825,000 908,000 770,000 -138,000

FY 2019 Funding by Subprogram

DOE/HEP PI Meeting 2018 48

HEP Funding Category ($ in K)

FY 2017 Actual

FY 2018 Enacted

FY 2019 Request

FY 19 vs. FY 18

Energy Frontier 154,274 190,938 181,232 -9,706

Intensity Frontier 242,924 246,768 200,170 -46,598

Cosmic Frontier 135,988 121,246 75,446 -45,800

Theoretical and Computational Physics

60,251 78,156 73,980 -4,176

Advanced Technology R&D 124,447 114,962 83,755 -31,207

Accelerator Stewardship 13,616 15,530 12,417 -3,113

Construction (Line Item) 93,500 140,400 143,000 +2,600

Total 825,000 908,000 770,000 -138,000

Research/Facilities/Project breakdown in following slides

Energy Frontier

Research: higher priority to support laboratory research activities to address the Higgs boson science driver, and to carry out the final analyses on data taken prior to LHC LS2 in 2019-20

Facility Operations: focus on commissioning of LHC ATLAS and CMS Detector Upgrade projects. Reduced support for compute nodes, data storage due to lower demand during LS2

Projects: increase supports new MIE starts for the HL-LHC ATLAS and HL-LHC CMS Detector Upgrade Projects and the planned increase for the HL LHC Accelerator Upgrade Project

DOE/HEP PI Meeting 2018 49

Energy Frontier($ in K)

FY 2017 Actual

FY 2018 Enacted

FY 2019 Request

FY 19 vs. FY 18

Research 72,268 79,530 56,119 -23,411

Facilities/Operations 52,771 54,340 44,309 -10,031

Projects 24,017 51,000 77,000 +26,000

LHC ATLAS Upgrade 8,500 - - ---

LHC CMS Upgrade 7,967 - - ---

HL-LHC Accelerator Upgrade 500 27,000 42,000 +15,000

HL-LHC ATLAS Upgrade 4,300 12,000 17,500 +5,500

HL-LHC CMS Upgrade 2,750 12,000 17,500 +5,500

SBIR/STTR 5,218 6,068 3,804 -2,264

Total 154,274 190,938 181,232 -9,706

Intensity Frontier

Research: higher priority to support laboratory research activities to address the neutrino mass and explore the unknown science drivers, and to carry out the early physics data analyses from Muon g-2, Belle II, SBN program and protoDUNE.

Facility Operations: activities will prioritize delivering the particle beams and providing experimental operations for ongoing experiments, including NOvA, SBN program, and Muon g-2. The Fermilab Accelerator Complex will be running at 75% of optimal levels.

Projects: focus on preliminary design and prototyping for the PIP-II project. OPC will continue for LBNF/DUNE for plant support costs.

DOE/HEP PI Meeting 2018 50

Intensity Frontier($ in K)

FY 2017 Actual

FY 2018 Enacted

FY 2019 Request

FY 19 vs. FY 18

Research 56,317 60,700 41,246 -19,454

Facilities/Operations 154,301 153,385 125,916 -27,469

Projects 24,569 24,100 26,000 +1,900

LBNF/DUNE - 1,000 1,000 ---

PIP-II 15,220 23,100 25,000 +1,900

Muon G-2 6,349 - - ---

SBIR/STTR 7,737 8,583 7,008 -1,575

Total 242,924 246,768 200,170 -46,598

Cosmic Frontier

Research: higher priority to support laboratory research activities to address the dark matter and dark energy science drivers, and to carry out the final data analyses on Cosmic Frontier experiments completing in FY 2019

Facility Operations: focus on the installation, commissioning and pre-operations activities for LSSTcam, DESI, LZ, and SuperCDMS-SNOLAB as these projects transition to operations

Projects: priority to support the fabrication and installation of the DESI, LZ, and SuperCDMS-SNOLAB projects. LSSTcam project funding will conclude as planned

DOE/HEP PI Meeting 2018 51

Cosmic Frontier($ in K)

FY 2017 Actual

FY 2018 Enacted

FY 2019 Request

FY 19 vs. FY 18

Research 45,990 49,892 31,506 -18,386

Facilities/Operations 13,353 16,310 11,320 -4,990

Projects 74,375 52,400 30,850 -21,550

LSSTcam 45,000 9,800 - -9,800

DESI 12,800 20,000 11,400 -8,600

LZ 12,500 14,100 14,450 +350

SuperCDMS 3,400 7,400 5,000 -2,400

SBIR/STTR 2,270 2,644 1,770 -874

Total 135,988 121,246 75,446 -45,800

Theoretical and Computational Physics

Theory Research: higher priority to research that addresses the neutrino mass science driver

Computational HEP: priority to advance computing research for HEP needs, and working with ASCR to optimize the high performance computing

Quantum Information Science: focus on research techniques and algorithms, foundational concepts relating particle physics and QIS, quantum computing for HEP experiments and modeling, development and use of specialized quantum controls and precision sensors

DOE/HEP PI Meeting 2018 52

Theoretical and Computational Physics($ in K)

FY 2017 Actual

FY 2018 Enacted

FY 2019 Request

FY 19 vs. FY 18

Research 55,713 75,303 71,280 -4,023

Theoretical Physics 44,848 43,000 32,753 -10,247

Computational HEP 7,924 8,500 7,435 -1,065

Quantum Information Science - 18,000 27,500 +9,500

Projects 2,300 - - ---

SBIR/STTR 2,238 2,853 2,700 -153

Total 60,251 78,156 73,980 -4,176

Advanced Technology R&D

General Accelerator R&D: priority to world-leading efforts supported at national laboratories

Directed Accelerator R&D: funding reduced as LARP goals will have been met

Detector R&D: near-term R&D activities will be ramped down

Facility Operations: focus on accelerator, test beam, and detector facilities at Fermilab. Funding for LBNL, SLAC supports highest priority research and fabrication activities. LBNL BELLA Second Beamline AIP begins, offset by completion of SLAC Sector 10 Injector Infrastructure AIP

Projects: focus on critical FACET-II infrastructure to be installed during shutdown for LCLS-II

DOE/HEP PI Meeting 2018 53

Advanced Technology R&D($ in K)

FY 2017 Actual

FY 2018 Enacted

FY 2019 Request

FY 19 vs. FY 18

Research 83,334 70,757 53,283 -17,474

GARD 44,357 44,500 36,544 -7,956

LARP 21,800 5,000 - -5,000

MAP 1,000 - - ---

Detector R&D 16,177 17,000 13,690 +9,500

Facilities/Operations 33,403 30,500 25,525 -4,975

Projects (FACET-II) 3,500 10,000 2,000 -8,000

SBIR/STTR 4,210 3,705 2,947 -758

Total 124,447 114,962 83,755 -31,207

Accelerator Stewardship

Research: priority will be given to long-term R&D for the science and technology needed to build future generations of accelerators.

Facility Operations: ATF II Upgrade AIP completion partially offset by the start of the 20TW CO2 Laser Upgrade AIP

DOE/HEP PI Meeting 2018 54

Accelerator Stewardship($ in K)

FY 2017 Actual

FY 2018 Enacted

FY 2019 Request

FY 19 vs. FY 18

Research 8,270 9,000 8,032 -968

Facilities/Operations 4,868 6,000 3,950 -2,050

SBIR/STTR 478 530 435 -95

Total 13,616 15,530 12,417 -3,113

Line Item Construction

LBNF/DUNE: funding will continue for far site civil

construction for the excavation of the caverns

Mu2e: FY 2019 will be last year of funding for the

project

PIP II: project engineering and design funding was

initiated in the FY 2018 enacted appropriation

DOE/HEP PI Meeting 2018 55

Construction (Line Item) ($ in K)

FY 2017 Actual

FY 2018 Enacted

FY 2019 Request

FY 19 vs. FY 18

LBNF/DUNE 50,000 95,000 113,000 +18,000

Mu2e 43,500 44,400 30,000 -14,400

PIP-II - 1,000 - -1,000

Total 93,500 140,400 143,000 +2,600

HEP MIE Project Status

DOE/HEP PI Meeting 2018 56

SubprogramTPC ($M)

CD Status

CD Date

INTENSITY FRONTIER

Long Baseline Neutrino Facility / Deep Underground Neutrino Experiment (LBNF/DUNE)

1,260 –1,860

CD-3A September 1, 2016

Proton Improvement Project (PIP-II) 653 - 928 CD-1 July 23, 2018

Muon g-2 44 CD-4 January 16, 2018

Muon-to-Electron Conversion Experiment (Mu2e) 274 CD-3 July 14, 2016

ENERGY FRONTIER

LHC ATLAS Detector Upgrade 33 CD-3 November 12, 2014

LHC CMS Detector Upgrade 33 CD-4A September 19, 2017

High-Luminosity LHC (HL-LHC) Accelerator Upgrade 208 - 252 CD-1/3A October 13, 2017

High-Luminosity LHC (HL-LHC) ATLAS Detector Upgrade 125-155 CD-0 April 13, 2016

High-Luminosity LHC (HL-LHC) CMS Detector Upgrade 125-155 CD-0 April 13, 2016

COSMIC FRONTIER

LUX-ZEPLIN (LZ) 56 CD-3 February 9, 2017

Super Cryogenic Dark Matter Search - SNOLAB (SuperCDMS-SNOLAB) 18.6 CD-2/3 May 2, 2018

Dark Energy Spectroscopic Instrument (DESI) 56 CD-3 June 22, 2016

Large Synoptic Survey Telescope Camera (LSSTcam) 168 CD-3 August 27, 2015

ADVANCED TECHNOLOGY R&D

Facility for Advanced Accelerator Experimental Tests II (FACET-II) 24.6 CD-2/3 June 8, 2018