EU Design

1
FAIR Facility for Antiproton and
Ion Research FP6 Proposals Status
and Recent Activities
Walter F. Henning / GSI Darmstadt
NuPECC, Lisbon, November 2004
2
FAIR - FP6 Proposals
3
FAIR Design Study Proposal

• Scope Design of accelerators and experiments
  with secondary beams at FAIR
• PANDA experiment (Hadron physics with
  antiprotons)
• NUSTAR experiment (Physics with radioactive
  beams)
• HESR (High Energy Storage Ring for cooled
  antiprotons)
• CR (Collector Ring Complex storage and cooler
  rings for RIB and antiprotons)
• SIS100 (Superconducting Synchrotron with 100 Tm)
• Participation 33 Institutes in Europe, USA,
  Russia
• Budget total budget 22 Mio ? EC support 9
  Mio
• Duration 36 month
• Status Evaluation passed successfully
• Start of contract negotiation with
  EC in August 2004
• Submission of Contract Preparation
  Forms and "Description of Work" (30.9.04)
• Preparation of Consortium Agreement

4
FAIR Construction Proposal

• Scope Construction of SIS18 upgrade including
  experiments
• SIS18 upgrade (to 4 Hz and lower charge state ?
  intensity increase factor 100)
• R3B magnet (Spectrometer magnet of reaction
  studies with RIB)
• HADES upgrade for high intensities and pion
  beams
• Participation 14 Institutes in Europe, USA,
  Russia
• Budget total budget 15 Mio ? EC support 15
  Mio ?
• Duration 48 month
• Status Letter from EC in August 2004
• Good evaluation result ? Funding
  depends on decision regarding 2. call
• Start of funding period in 2006 ?

5
Accelerator Physics and Technology for FAIRMain
RD challenges
Superconducting, fast ramping synchrotron magnets
High gradient, low frequency RF cavities
Novel lattice/collimation design Beam optics
studies
SIS 100 dipole magnet
control of stripping losses
CR compressor cavity
Control of collective effects Large scale
simulation studies
Ultra high vacuum for intense beams
Fast stochastic and electron cooling
Working point diagram Stability of intense beams
Desorption test-stand
HESR e-cooler
6
FAIR - Status and Recent Activities
7
The Future International Facility at GSI
FAIR - Facility for Antiproton and Ion
Research
Existing
Future Project
100 m
8
The Future International Facility at GSI
FAIR - Facility for Antiproton and Ion
Research
Existing
Future Project
Beams in the future Intensity 100 1000 fold
Species Z -1 92 (anti-protons to uranium)
Energies up to 35 - 45 GeV/u Precision beam
cooling
Beams now Z 1 92 (protons to uranium) up
to 2 GeV/nucleon Beam cooling
100 m
9
The FAIR Project
SIS 100
SIS 300

• Nuclear Structure Physics and
• Nuclear Astrophysics with
• Radioactive Ion-Beams
• Hadron Physics with Antiprotons
• Physics of Nuclear Matter with
• Relativistic Nuclear Collisions
• Plasma Physics with Highly
• Bunched Laser- and Ion-Beams
• Atomic Physics, Fundamental
• Symmetries and Applied Sciences
• Accelerator Physics

GSI today
SIS18 Upgrade
Beamlines
CBM
Antiproton Production Target
Plasma Phys.
Atom.Phys.
PANDA
El.Cooler
High En. Expt.
Low En. Expt.
FLAIR
NESR Expts
10
The FAIR Project
SIS 100
SIS 300

• Nuclear Structure Physics and
• Nuclear Astrophysics with
• Radioactive Ion-Beams
• (IFF not ISOL ?? EURISOL)
• Hadron Physics with Antiprotons
• (not rare K-decays neutrinos ?? J-PARC)
• Physics of Nuclear Matter with
• Relativistic Nuclear Collisions
• (High-density regime ?? RHIC, LHC)
• Plasma Physics with Highly
• Bunched Laser- and Ion-Beams
• (Dense, strongly coupled plasma ?? MCP)
• Atomic Physics, Fundamental
• Symmetries and Applied Sciences
• (Naked atoms anti-matter ?? EBIS, AD)
• Accelerator Physics
• (High-current synchrotrons and storage rings

GSI today
SIS18 Upgrade
Beamlines
CBM
Antiproton Production Target
Plasma Phys.
Atom.Phys.
PANDA
El.Cooler
High En. Expt.
Low En. Expt.
FLAIR
NESR Expts
11
FAIR - Recent Organizational Developments
12
FAIR - The 3-Stage Construction Scenario
13
2006 2007 2008 2009 2010 201 2012 2013 2014

2005
2006
2007
2008
2009
2010
2011
2012
2013
SIS18 Upgrade

70 MW Connection
Proton-Linac

General Planning
2,7x1011 /s 238U28 (200 MeV/u) 5x1012 protons
per puls
I
Civil Construction 1
SIS100/300 Tunnel, SIS InjectionExtractionTransf
er
SIS100 Transfer Line SIS18-SIS100 High Energy
Beam Lines
Transfer Buildings/Line Super-FRS, Auxiliary
Bldgs., Transfer Tunnel to SIS18, Building APT,
Super-FRS, CR-Complex RIB HighLow Energy Branch,
II
Civil Construction 2
RIB Prod.-Target, Super-FRS RIB HighLow Energy
Branch Antiproton Prod.-Target CR-Complex
1x1011/s 238U28 (0.4-2.7GeV/u) -gtRIB (50 duty
cycle) 2.5x1013 p (1-30 GeV) 3-30 GeV pbar-gtfixed
target 10.7 GeV/u 238U -gt HADES
III
Civil Construction 3
CBM-Cave, Pbar-Cave, Reinjection SIS100
HESR . 4 MV e- Cooling In NESR
IV
HESR ( ground level), NESR, AP-cave, e-A
Collider, PP-cave
Accuracy 6 -8 months
Civil Construction 4
SIS300 8 MV e- Cooling e-A Collider
1x1012/s 238U28 100 duty cycle pbar cooled p
(1-90 GeV) 35 GeV/u 238U92 NESR physics plasma
physics
V

Civil Construction


Experiment Potential
Civil Construction
Production and Installation
SIS300 installation together with SIS100
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Advanced Staging Scenario

• General strategy
• Groundwork, supply systems and major buildings as
  early as financially possible
• (potential for smoothing financial
  profile?)
• Scientific facilities staged according to three
  physics programmes
• Contributions from outside mainly in-kind for
  scientific facilities (?)

15
Advanced Staging Scenario

• Three stages according to different fields of
  research
• Radioactive ('Rare Isotope') Beams for
• Nuclear structure and nuclear astrophysics
• Atomic physics studies with highly
  charged/radioactive ions
• Proton-Antiproton Physics
• QCD studies with proton and antiproton beams
• precision studies with antiprotons addressing
  fundamental symmetries and interactions
• Final facility
• Full parallel operation of up to four research
  programs
• Full energy and luminosity for nuclear collisions
  program at CBM
• Precision QCD Studies at PANDA up to 15 GeV
• Plasma research (full gain factor in power
  density 400)
• Atomic reaction studies with fast beams

16

• Civil Construction
• Ringtunnel for double ring synchrotron incl.
  technical buildings
• Buildings housing the SFRS, the CR and NESR plus
  nuclear structure and atomic physics experiments
• Office building
• Accelerator
• 2 x 1011/puls U28 at 200 AMeV
• 4 x 1010/puls U73 at 1000 AMeV
• 4 Hz up to 12 Tm 1 Hz up to 18 Tm
• Bunch compression to 70 ns
• Research
• Nuclear structure and nuclear astrophysics (gain
  factor in intensities for radioactive secondary
  beams 100)
• Plasma physics at 'old' facility
• (gain factor in power density 200)
• Atomic physics studies with highly
  charged/radioactive ion beams

Stage 1
17

• Civil Construction
• Ringtunnel for double ring synchrotron incl.
  technical buildings
• Buildings housing the SFRS, the CR and NESR plus
  nuclear structure and atomic physics experiments
• Office building
• Accelerator
• 2 x 1011/puls U28 at 200 AMeV
• 4 x 1010/puls U73 at 1000 AMeV
• 4 Hz up to 12 Tm 1 Hz up to 18 Tm
• Bunch compression to 70 ns
• Research
• Nuclear structure and nuclear astrophysics (gain
  factor in intensities for radioactive secondary
  beams 100)
• Plasma physics at 'old' facility
• (gain factor in power density 200)
• Atomic physics studies with highly
  charged/radioactive ion beams

Stage 1
18

• Civil Construction (completion)
• p linac building
• HESR building
• Buildings housing nuclear collision, plasma
  physics and atomic physics experiments
• Accelerator
• 1 x 1012/puls U28 at 2,7 AGeV
• 1 x 1011/puls U73 at 8,3 AGeV (Ne10 bis 14
  AGeV)
• Bunch compression to 50 ns
• 2,5 x 1013/puls protons up to 29 GeV
• up to 1011 antiprotons accumulated, stored and
  cooled in the HESR up to 15 GeV
• low (down to zero) energy antiprotons at NESR and
  HITRAP
• Research
• Nuclear structure and nuclear astrophysics (full
  gain factor in intensities for radioactive
  secondary beams 1000-10000)
• QCD studies with cooled high-energy antiprotons
  (and protons)
• Precision studies with antiprotons addressing
  fundamental symmetries and interactions

Stage 2
HESR
19

• Civil Construction (completion)
• p linac building
• HESR building
• Buildings housing nuclear collision, plasma
  physics and atomic physics experiments
• Accelerator
• 1 x 1012/puls U28 at 2,7 AGeV
• 1 x 1011/puls U73 at 8,3 AGeV (Ne10 bis 14
  AGeV)
• Bunch compression to 50 ns
• 2,5 x 1013/puls protons up to 29 GeV
• up to 1011 antiprotons accumulated, stored and
  cooled in the HESR up to 15 GeV
• low (down to zero) energy antiprotons at NESR and
  HITRAP
• Research
• Nuclear structure and nuclear astrophysics (full
  gain factor in intensities for radioactive
  secondary beams 1000-10000)
• QCD studies with cooled high-energy antiprotons
  (and protons)
• Precision studies with antiprotons addressing
  fundamental symmetries and interactions

Stage 2
HESR
20
Stage 3

• Accelerator
• 2 x 109/puls U92 up to 34 AGeV
• Stretcher option with long extraction times from
  seconds up to minutes
• High energy e-cooling for HESR
• Research
• Full energy and luminosity for high-density
  nuclear matter program at CBM
• Precision QCD Studies at PANDA up to 15 GeV
• Plasma research (full gain factor in power
  density 2500)
• Atomic reaction studies with fast beams
• Full parallel operation of up to four research
  programs

21
Stage 3

• Accelerator
• 2 x 109/puls U92 up to 34 AGeV
• Stretcher option with long extraction times from
  seconds up to minutes
• High energy e-cooling for HESR
• Research
• Full energy and luminosity for high-density
  nuclear matter program at CBM
• Precision QCD Studies at PANDA up to 15 GeV
• Plasma research (full gain factor in power
  density 2500)
• Atomic reaction studies with fast beams
• Full parallel operation of up to four research
  programs

22
Some Considerations Concerning a Financial Plan
23
Cost Profile for Stages 1 - 2 - 3
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25
International Coordination and Legal Structure of
FAIR
26
International Committee Structure for
theFacility for Antiproton and Ion Research
(FAIR)
International Steering Committee
(ISC-FAIR) H. Schunck
Working Group on Administrative and Financial
Issues (AFI-FAIR) H-F. Wagner
Working Group on Scientific and Technical
Issues (STI-FAIR) S. Gales
27
International Committee Structure for
theFacility for Antiproton and Ion Research
(FAIR)
International Steering Committee
(ISC-FAIR) H. Schunck
Working Group on Administrative and Financial
Issues (AFI-FAIR) H-F. Wagner
Working Group on Scientific and Technical
Issues (STI-FAIR) S. Gales
LoI Submission (1800 authors) Jan. 15 April
15, 2004 PAC Meeting June 14-16, 2004
PAC / QCD R. Chiavassa
PAC / NSTR R. Casten
PAC / APPA D. Schwalm
TAC / ACC Y. Cho
28
International Committee Structure for
theFacility for Antiproton and Ion Research
(FAIR)
International Steering Committee
(ISC-FAIR) H. Schunck
Working Group on Administrative and Financial
Issues (AFI-FAIR) H-F. Wagner
Working Group on Scientific and Technical
Issues (STI-FAIR) S. Gales
Financial Plan Cost Attribution
Cost Estimates Controlling
29
Signing of MoU
AFI
Phase II Governed by contracts
MoU
Phase I Governed by MoU
Contract Development
Contract Negotiations
Closing
2004
2005
2006
STI
LoI's
Proposals / TR's
TDR's
Technical Committee
PAC's
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The International Steering Committee for FAIR
ISC Internat. Steering Committee H.Schunck
STI Working Group Scientific Technical
Issues Sidney Gales
AFI Working Group Administrative and
Funding Issues H.-F.Wagner
FAIR Project
PAC QCD E.Chiavassa
PAC NUSTAR R.Casten
PAC APPA D.Schwalm
TAC Yanglai Cho
EU
Observers
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FAIR Organisational Structure EEIG
Finland / France / Italy / Germany / Spain /
Sweden / UK ...Russia...Cons...
Council EEIG (Representatives of Partners)
Finland
GSI
France
Project Management
Italy
FAIR Project EEIG
Spain
Sweden
UK
...
Poland
Russia

...
...
Consort.
Observer
Requests of the Project from the partners, GSI
and external
Resources, Finances, Manpower and Hardware
Contributions
32
FAIR Organisational Structure EEIG
Finland / France / Italy / Germany / Spain /
Sweden / UK ...Russia...Cons...
Council EEIG (Representatives of Partners)
Finland
GSI
France
Project Management
DG
Italy
FAIR Project EEIG
ADR ADA ADI ADF ADFP
Spain
Sweden
Research
Accelerator
UK
Infrastructure
...
Administration
Poland
Russia
Future Project

...
...
Consort.
Observer
Requests of the Project from the partners, GSI
and external
Resources, Finances, Manpower and Hardware
Contributions
33
FAIR Organisational Structure GmbH
Finland / France / Italy / Germany / Spain /
Sweden / UK ...Russia...Cons...
Council (Representatives of Partners)
Finland
GSI
France
Project Management
Italy
FAIR Project GmbH
Spain
Sweden
UK
...
Poland
Russia

...
...
Consort.
Observer
Requests of the Project from the partners, GSI
and external
Resources, Finances, Manpower and Hardware
Contributions
34
FAIR Organisational Structure GmbH
Finland / France / Italy / Germany / Spain /
Sweden / UK ...Russia...Cons...
Council (Representatives of Partners)
Finland
GSI
France
Project Management
Italy
?
FAIR Project GmbH
Spain
Sweden
UK
...
Poland
Russia

...
...
Consort.
Observer
Requests of the Project from the partners, GSI
and external
Resources, Finances, Manpower and Hardware
Contributions
35
FAIR as a German Limited Liability Company with
International Shareholders
International Steering Commitee
Administration and Financial Issues WG
Fair Project Group
Scientific and Technical Issues WG
Operations
FAIR
36
FAIR as a German Limited Liability Company with
International Shareholders
International Steering Commitee
Administration and Financial Issues WG
Scientific and Technical Issues WG
Articles of Association (Charter) Consortial
Agreement (Memoranda of Understanding)
37
Host-Laboratory Activities
38
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39
Legal and Regulatory Procedures for Construction
Planning of FAIR
40
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41
(No Transcript)
42
Radiation Safety Approval Procedure
In February 2002, one year before the green
light was obtained from the German government,
GSI applied for the Construction of an
International Facility for the Research with Ion
and Proton Beams at the Hessian Ministry for
Environment
In December 2003, GSI received official letter
with the first approval ....the planned
facility will fulfill the requirements in
accordance with the German radiation protection
laws for the construction of the whole
installation and the operation as outlined in the
Conceptual Design Report.
43
FAIR - Two Brief Remarks on Physics Aspects
44
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45
Giant resonances in exotic nuclei

• In-medium interactions isospin effects (dipole
  res. ?? sym.energy)
• strong fragmentation
• spreading width in n-rich nuclei ?
• new coherent modes (diff. proton-neutron
  deformation)
• Soft excitation modes
• Pygmy Dipole Resonance
• Astrophysics implications

46
Production of exotic nuclear beams by
fragmentation
advantage shortlived isotopes (T1/2lt ms)
accessible
About 1000 nuclear residues identified
132Sn
Land Collaboration P. Adrich et al., 2004
A/Z-resolution 10-3
47
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