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FAIR – F acility for A ntiproton and I on R esearch * FP6 Proposals

FAIR – F acility for A ntiproton and I on R esearch * FP6 Proposals * Status and Recent Activities Walter F. Henning / GSI Darmstadt NuPECC, Lisbon, November 2004. FAIR - FP6 Proposals. FAIR Design Study Proposal.

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FAIR – F acility for A ntiproton and I on R esearch * FP6 Proposals

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  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 • Signing of contract with EC end 2004 / beginning 2005 • Start of funding period Spring 2005

  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 R&D challenges High gradient, low frequency RF cavities Novel lattice/collimation design: Beam optics studies Superconducting, fast ramping synchrotron magnets control of stripping losses SIS 100 dipole magnet 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. SIS 100/300 SIS UNILAC FRS ESR HESR Super FRS CR NESR RESR The Future International Facility at GSI:FAIR - Facility for Antiproton and Ion Research Existing Future Project 100 m

  8. SIS 100/300 SIS UNILAC FRS ESR HESR Super FRS CR NESR RESR 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. SIS UNILAC FRS ESR HESR Super FRS CR NESR RESR 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. SIS UNILAC FRS ESR HESR Super FRS CR NESR RESR 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. 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 Injection+Extraction+Transfer 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 High+Low Energy Branch, II Civil Construction 2 RIB Prod.-Target, Super-FRS RIB High+Low Energy Branch Antiproton Prod.-Target CR-Complex 1x1011/s 238U28+ (0.4-2.7GeV/u) ->RIB (50% duty cycle) 2.5x1013 p (1-30 GeV) 3-30 GeV pbar->fixed target 10.7 GeV/u 238U -> 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

  14. 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 physicsat '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

  24. International Coordination and Legal Structure of FAIR

  25. 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

  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 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

  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 Cost Estimates & Controlling Financial Plan & Cost Attribution

  28. ~ 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

  29. 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:

  30. 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 … ... ... Observer Consort. Requests of the Project from the partners, GSI and external Resources, Finances, Manpower and Hardware Contributions

  31. 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 … ... ... Observer Consort. Requests of the Project from the partners, GSI and external Resources, Finances, Manpower and Hardware Contributions

  32. 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 … ... ... Observer Consort. 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 … ... ... Observer Consort. Requests of the Project from the partners, GSI and external Resources, Finances, Manpower and Hardware Contributions

  34. 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

  35. 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)

  36. Host-Laboratory Activities

  37. Legal and Regulatory Procedures for Construction Planning of FAIR

  38. 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 letterwith 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.

  39. FAIR - Two Brief Remarks on Physics Aspects

  40. 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

  41. 1GeV/u U + H Production of exotic nuclear beams by fragmentation advantage: shortlived isotopes (T1/2< ms) accessible About 1000 nuclear residues identified 132Sn Land Collaboration P. Adrich et al., 2004 A/Z-resolution ~10-3

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