Facility for Antiproton and Ions Research

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FAIR Project – status and research program Zbigniew Majka – FAIR Joint Core Team, Head of Research

Facility for Antiproton and Ions Research

Helmholtz Centre for Ion Research

Zbigniew Majka

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GmbHGmbH

Future facilityFuture facility

GSI todayGSI todayMarch 2007

Locations preparation for deep hole drilling(for soil analysis)

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Spring 2006

STI presented FAIR Baseline Technical Report - 2400 authors

Late 1990sGSI researchers began discussion with the 1200 outside users

2001 GSI had drawn up the Conceptual Design Report for a new facility

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Facility for Antiproton and Ions Research project - has been developed by

an international science community and

the Hemholtz Association’s Research Center GSI in Darmstadt

Zbigniew Majka

will be constructed over the next eight years and

will provide scientists from various fields of research with unprecedented high-quality beams

of both stable and unstable nuclei as well as of antiprotonsin a wide range of intensities and energies

for a multifaceted, multidisciplinary forefront science programme.

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Construction Period, Cost, Users

Commissioning Costs 28 M€ Operation Costs up to 2025 1485 M€

Construction until 2016 Total cost 1.2 B€Scientific users: 2500 - 3000 per year

Financing

up to 65 % Federal Government of Germany 10 % State of Hessen 25 % Partner Countries

FAIR GmbH with

International Shareholders

Operation

Project Costs scrutinized by CORE, TAC, STI …as basis how to account in-kind contributions

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From Summary Record of 8th ISC Meeting, July 24, 2006, Berlin: “To the FAIR core facility belong the experiments of the 14 approved technical proposals (see table).”

Very diverse and ambitious program!

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T[K]

1 TeV 1016

1 GeV 1013

1 MeV 1010

1 KeV 107

1 eV 104

1 meV 10

10-12 10-6 1 106 1012 1018 t[s]

Quar-gluon souplept., neutr., fot., graw.,

Parlicles Nuclei

Atoms

Today15 bln y. later

FAIR – QCD research programs (Quantum Chromodynamics and Hadron Physics)

FAIR Research

George Gamov Fred Hoyle

The evolution of the universe

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FAIR SynchrotronsSIS100 and SIS300

GSI SynchrotronSIS18

GSI LinearAccelerator

p-Linac

HighEnergyStorageRing

CollectorRing AccumulatorRing RESR New

ExperimentalStorageRing

Antiproton Production TargetUnique features:e- cooling StorageIn-ring experiments

Ring [m] [Tm] [GeV] Ion/ Antip Radioactive

SIS100 1084 100 2.7 A (U28+), 29 p 2 10∙ 11/pulse 4 10∙ 13protons/pulse 5 10∙ 11 U /pulse

SIS300 1084 300 34 A (U92+), 2 10∙ 9/s

CR 211 13 0.74, A (U92+), 3 antip Fast stoch. cooling Fast stoch. cooling

RESR 245 13 0.74, A (U92+), 3 antip Accumul. of antip 1T/s decelerat .of short lived

NESR 222 13 0.74, A (U92+), 3 antip 1T/s decelerat .of antip 1T/s decelerat .of short lived, el. cool

HESR 574 50 14 GeV antip 0.8-14 GeV antip

Primary beam USIS100 + SIS300

x100-1000 over present intensityCBM

PANDA

FAIR Research – QCD

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FAIR Research – QCD/PANDA

Hadron Structure, QCD-Vacuum and Medium Stored and cooled antiprotons up to 15 GeV/c, ~ 520 users

See talks by: Zoltan Gagyl-Palffy - Physics with PANDA Detector at FAIR Marco Maggiora - Transvers Spin Physics at FAIR

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FAIR Research – QCD/CBM QCD-Phase Diagram: Nuclear & QGP Matter HI beams 2 to 45 GeV/u; ~ 390 usersBaryon density in central cell (Au+Au, b=0 fm): HSD: mean field, hadrons + resonances + strings QGSM: Cascade, hadrons + resonances + stringsC. Fuchs, E. Bratkovskaya, W. Cassing

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FAIR Research – QCD/CBM

Probing the equation-of-state at high B

Observables: collective flow of hadrons, particle production at threshold energies (open charm)

Search for a deconfined phase at high B enhanced strangeness production ? Observables: K, , , , anomalous charmonium suppression ? Observables: charmonium (J/ψ, ψ'), open charm (D0, D)

Search for chiral symmetry restoration at high B

in-medium modifications of hadrons Observables: , , e+e- , open charm, .....

Search for the 1. order phase transition & its critical endpoint Observable: event-by-event fluctuations (K/π, pT, ...)


T[K]

1 TeV 1016

1 GeV 1013

1 MeV 1010

1 KeV 107

1 eV 104

1 meV 10

10-12 10-6 1 106 1012 1018 t[s]


Parlicles Nuclei

Atoms

Sun5 bln y. ago


FAIR – NUSTAR research programs (Nuclear Structure, Astrophysics and Reactions

FAIR Research -NuSTAR

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FAIR SynchrotronsSIS100 and SIS300

GSI SynchrotronSIS18

GSI LinearAccelerator

p-Linac

HighEnergyStorageRing

CollectorRing AccumulatorRing RESR New

ExperimentalStorageRing

SuperFragmentSeparator Rare Isotopes

Production TargetSecondary beam;

High precision RIB up to 1.5 - 2 AGeV; x 10 000

Ring [m] [Tm] [GeV] Ion/ Antip Radioactive

SIS100 1084 100 2.7 A (U28+), 29 p 2 10∙ 11/pulse 4 10∙ 13protons/pulse 5 10∙ 11 U /pulse

SIS300 1084 300 34 A (U92+), 2 10∙ 9/s

CR 211 13 0.74, A (U92+), 3 antip Fast stoch. cooling Fast stoch. cooling

RESR 245 13 0.74, A (U92+), 3 antip Accumul. of antip 1T/s decelerat .of short lived

NESR 222 13 0.74, A (U92+), 3 antip 1T/s decelerat .of antip 1T/s decelerat .of short lived, el. cool

HESR 574 50 14 GeV antip 0.8-14 GeV antip

Primary beam USIS100 + SIS300

x100-1000 over present intensity


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Primary Beams

• 5.1011/s; 1.5-2 GeV/u; 238U28+

• Factor 100-1000

Secondary Beams

• up to factor 10 000SUPERconducting FRagment Separator

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FAIR Research - NuSTAR

Long Standing Questions of Nuclear Structure Physics

What are the limits for existence of nuclei?Where are the proton and neutron drip lines situated? Where does the nuclear chart end?

How does the nuclear force depend on varying proton-to-neutron ratios?What is the isospin dependence of the spin-orbit force?How does shell structure change far away from stability?

How to explain collective phenomena from individual motion?What are the phases, relevant degrees of freedom, and symmetries of the nuclear many-body system?

How are complex nuclei built from their basic constituents?What is the effective nucleon-nucleon interaction?How does QCD constrain its parameters?

Which are the nuclei relevant for astrophysical processes and what are their properties?

What is the origin of the heavy elements?


T[K]

1 TeV 1016

1 GeV 1013

1 MeV 1010

1 KeV 107

1 eV 104

1 meV 10

10-12 10-6 1 106 1012 1018 t[s]


Parlicles Nuclei

Atoms

Sun5 bln y. ago


FAIR – APPA research programs(Atomic ,Plasma Physics and Applications)

FAIR Research - APPA

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SPARC

FLAIR

WDMHEDgeHOB


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Physics of Dense Bulk Plasmas Ion-beam bunch compression & high-energy petawatt-laser; ~ 250 users

Fundamental Symmetries & Ultra-High EM Fields Antiprotons and highly stripped ions; ca. 250 users

Materials Science and Radiation Biology, etc. Ion & antiproton(?) beams; ~ 350 users


Radioactive Ion Beam Programme Anti Proton Beam Programme

Relat. Ion Beam ProgrammePlasma Physics Beam Programme


FAIR – Planned Experimental FacilitiesFAIR – Planned Experimental Facilities

100 m

UNILACSIS 18

SIS 100/300

HESR

SuperFRS

NESR

CR

RESR

ESR


Pictures from meetings (about 50/year) of the different experiment collaborations

CBM in StrasbourgCBM in Strasbourg

BIOMAT bei GSI SPARC in Poland

PANDA bei GSI

NUSTAR bei GSI

SPARC in PIASKI

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Confirmed international contributions

Total EU support for FAIR related activities in FP6: >32 M€

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EU-6FP-CNI: FAIR injector SIS18 intensity upgrade, HADES upgrade + R3BmagnetEU-Support: 10,4 M€

EU-6FP-Design Study: Secondary Beams (RIB and Antiprotons)EU-Support: 9 M€

EU-6FP-I3 programmes I3HadronPhysics: FAIR related EU-Support: 10,8 M€ EURONS: FAIR related EU-Support: 2 M€

plus 4,9 M€ in FP7 FAIR preparatory phase

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Call for EoIs sent out O

ctober 10th, 2007

21 Expression of Interests received so far !

25Zbigniew Majka QuickTime™ and aTIFF (Uncompressed) decompressor

are needed to see this picture.

EoIs still missing from

All information can be found on the WEB page

http://www-win.gsi.de/FAIR-EOI/

http://www-win.gsi.de/FAIR-EOI/

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• Accelerator Developments

Fast ramping:Frequency variable ferrite or MA loaded resonators

Beam quality:Electron & Stochastic Cooling

XHV ~10-12 mbar

Compact & efficient acceleator design:Rapidly cycling sc magnets: dB/dt ~ 4T/s

http://www.hochschule-fulda.de/index.php?id=134

FAIR Start Event, November 7/ 8, 2007

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1400 international participants 500 international scientists attended the symposium on the Physics of FAIR

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Draft-Schedule

Start of operation in 2013-2015 is feasible, provided we start mid 2008.

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The ISC is confident, that the FAIR Convention Signing Conference can take place in late autumn this year

and FAIR GmbH will be established

17th Meeting of the FAIR-International Steering Committee

July 4, 2008, 9:30 – 17:00 h at GSI, Darmstadt, Germany

The next meeting of the FAIR Steering Committee is scheduled

on Wednesday September 3rd, 2008 at GSI, Darmstadt.

Recruitment of the FAIR Scientific Director – has high priority, Job advertisement was published in the following journals or newspapers: CERN Courier , Physics Today , Nupecc News , German and US newspaper,

recruitment of the Administrative Director will be postponed to allow the Scientific Director to get involved

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Austria

China

Finland

Germany Hessen India

Poland Romania Russia Spain Sweden

UKSlovenia

Facility for Antiproton and Ion Research

FAIR = International Accelerator Facility 'next' to GSI

Shares not yet defined

Thank you !

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KoscieliskoKoscielisko

Documents

Facility for Antiproton and Ions Research