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Status of the FAIR project at GSI, Darmstadt International TRD workshop Romania, September 24-28, 2005 J. Eschke, GSI. Overview of the FAIR Facility Status evaluation of scientific program and technical planning of accelerators Roadmap of International Steering Committee
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Status of the FAIR project at GSI, Darmstadt International TRD workshop Romania, September 24-28, 2005 J. Eschke, GSI Overview of the FAIR Facility Status evaluation of scientific program and technical planning of accelerators Roadmap of International Steering Committee 4. Next Steps
Key Technical Features • Cooled beams • Rapidly cycling superconducting magnets International FAIR Project:Facility Characteristics Primary Beams • 1012/s; 1.5-2 GeV/u; 238U28+ • Factor 100-1000 over present intensity • 2(4)x1013/s 30 GeV protons • 1010/s 238U92+ up to 35 GeV/u • up to 90 GeV protons SIS 100/300 SIS UNILAC FRS Secondary Beams ESR • Broad range of radioactive beams up to 1.5 - 2 GeV/u; up to factor 10 000 in • intensity over present • Antiprotons 0 - 30 GeV HESR Super FRS Storage and Cooler Rings CR NESR FLAIR • Radioactive beams • e- – A (or Antiproton-A) collider • 1011 stored and cooled 0.8 - 14.5 GeV antiprotons • Polarized antiprotons(?) RESR
Five Scientific Pillars • Research Areas: • Nuclear structure and nuclear astro- • physics with beams of short-lived nuclei • Hadron physics and QCD with cooled • antiproton beams • Physics of high-density nuclear matter • and the quark-gluon phase transition • Physics of dense plasmas • Atomic physics, fundamental symmetries • and material science How are the elements from Iron to Uranium made ? What is Mass? (and polarisation) Mass in Medium? Interior of Stars and Planets Highest EM Fields, exotic nuclei, exotic atoms, anti-matter, (antimatter)
Nuclear structure and nuclear astro-physics with beams of short-lived nuclei Isotopes accessible by the Super-FRS FAIR
NUSTAR Technical Proposals • The NUSTAR Community 600 people from about 70 Institutions In-Flight Radioactive Beam Facility (0 - 1500 AMeV) High intensity primary beams (e.g. 1012238U / sec at 1 GeV/u)
detector features: measurement and identification of , e , , , K, p, p high rate capability fast trigger scheme High-Energy Storage & Cooler Ring (HESR) und Detector p-injection HESR electron cooler universal detector PANDA circumference 442 m max. bending power 50 Tm p
Physics Potential of the Antiproton Facility glueballs (ggg) hybrids (ccg) p momentum [GeV/c] J/ spectroscopy confinement hidden and open charm in nuclei fundamental symmetries: p in traps (FLAIR) strange and charmed baryons in nuclear field Light Mesons Charmonium Mass [GeV/c2] • Quark gluon structure and dynamics of “strong” interacting particles; • Origin of the confinement and mass of hadron
CBM ECAL (12 m) TOF (10 m) TRDs (4,6,8 m) RICH (1,5 m) STS (5 – 100 cm) beam magnet Physics of Nuclear Matter Studies with Relativistic Nuclear Collisions • Studies of hadronic matter at high net baryon densities; • Phase transitions in quark matter at large µB • in-medium mass modification in dense matter
Since mid 90ies: Concrete ideas about GSI's future 2000: First draft of an 'International accelerator centre for research with antiproton and ion beams' Autumn 2001: Conceptual Design Report 2002: Evaluation by the Science Council of Germany (together with 8 other big projects) Positive Recommendation, but: Extension in Stages (Stage Planning) At least 25% of the investment cost of 675 M€ has to be raised from international partners. Feb. 5th, 2003: Positive decision of the ministry for education and research of Germany History of the FAIR project
Administrative: Feb. 2004: Establishment of the International Steering Committee (ISC)Subcommittees: AFI (Administrative and Funding Issues) STI (Scientific and Technical Issues) September 2004: Memorandum of Understanding Scientific: Spring 2004: Submission of 25 Letters of Intent(partially experiments in addition to the original CDR, e.g. FLAIR, PAX) January 2005: 21 Collaborations submit Technical Proposals and 14 Technical Reports for the accelerator and infrastructure History of the FAIR project (2)
The International Steering Committee for FAIR ISC Internat. Steering Committee H. Schunck AFI Working Group Administrative and Funding Issues H.-F. Wagner STI Working Group Scientific + Technical Issues H. Wenninger FAIR Project PAC QCD E.Chiavassa Legal Working Group U. Jahn PAC NUSTAR R.Casten PAC APPA D.Schwalm Full Cost Issues Group B. Brandt TAC Yanglai Cho Cost Review Group 'E' ExperimentsW. Bartel Cost Review Group 'A' Accelerators D. Plane Observers:
Status Signatures Memorandum of Understanding for the FAIR project (January 18, 2005) Observers: EU, USA, China, Hungary, India, Austria China and India intent to sign the MoU Romania declared to become observer in the ISC
The International Steering Committee for FAIR ISC Internat. Steering Committee H. Schunck AFI Working Group Administrative and Funding Issues H.-F. Wagner STI Working Group Scientific + Technical Issues H. Wenninger FAIR Project PAC QCD E.Chiavassa Legal Working Group U. Jahn PAC NUSTAR R.Casten PAC APPA D.Schwalm Full Cost Issues Group B. Brandt TAC Yanglai Cho Cost Review Group 'E' ExperimentsW. Bartel Cost Review Group 'A' Accelerators D. Plane Observers:
Technical Proposals (TP) following last year’s LoIs PAC on Nuclear Structure and Nuclear Astrophysics (NUSTAR-PAC): 1.) Low Energy Branch (LEB) High-resolution In-Flight Spectroscopy (HISPEC)/ Zs.Podolyak/ Surrey Decay Spectroscopy with Implanted Ion Beams (DESPEC) + B. Rubio Valencia Precision Measurements of very short-lived Nuclei using an Advanced Trapping System for highly-charged Ions (MATS) K.Blaum Mainz LASER Spectroscopy for the Study of Nuclear Properties (LASPEC) P. Campbell Manchester Neutron Capture Measurements (NCAP) M.Heil FZK Antiprotonic Radioactive Nuclides (Exo+pbar) M. Wada Riken 2.) High Energy Branch (R3B) A Universal Setup for Kinematical Complete Measurements of Reactions with Relativistic Radioactive Beams (R3B) T. Aumann GSI 3.) Ring Branch (STORIB) Study of Isomeric Beams, Lifetimes and Masses (ILIMA) Y .Novikov SPNPI Exotic Nuclei Studied in Light-Ion Induced Reactions at the NESR Storage Ring (EXL) M. Chartier Liverpool Electron-Ion Scattering in a Storage Ring (e-A Collider) (ELISe) H. Simon GSI Antiproton-Ion Collider: A Tool for the Measurement of Neutron and Proton rms radii of Stable and Radioactive Nuclei (AIC) R. Krücken TUM Spectroscopy of Pionic Atoms with Unstable Nuclei (PIONIC) K. Itahashi Riken 667 users in 10 TP
Technical Proposals (TP) following last year’s LoIs 909 users in 4 TPs PAC on QCD: (ASSIA Study of Spin-dependent Interactions with Antiprotons) R.Bertini Torino CBM Compressed Baryonic Matter Experiment P.Senger GSI PANDA Strong Interaction Studies with Antiprotons U.Wiedner TSL Uppsala PAX Antiproton-Proton Scattering Experiments with Polarization F.Rathmann FZJ PAC on Atomic Physics, Plasma Physics and Applications (APPA-PAC): Laser Cooling of Highly Charged Ions at SIS 100/300 U. Schramm LMU FLAIR - A Facility for Low-energy Antiproton and Ion Research E. Wiedman Tokyo SPARC Stored Particles in Atomic physics Research R. Schuch Stockholm HEDGEHOB: High Energy Density matter GEenerated by Heavy-iOn Beams D. Varentsov Darmstadt Applications of Relativistic Ions in Radiobiology and Space Research M. Durante Napoli Materials Research with Relativistic Heavy Ion Beams S. Klaumünzer HMI Radiative Properties of Warm Dense Matter F. B. Rosmej Marseille 578 users in 5 TPs
Recommendations of the STI Working Group on FAIR • 13 Technical Proposals approved • 3 Technical Proposals rejected • 2 Proposal considered as 2nd generation experiments • (to be worked out in detail) Experiment cost evaluation by Cost Review Commmittee (CoRe E) performed for: CBM, PANDA, SPARC, R3B, MATS, LASPEC,ILIMA, HISPEC/DESPEC
FAIR Layout January 2005 Technical Reports • SIS18 upgrade • SIS100 • SIS300 • Super-FSR • CR • RESR • NESR • Proton LINAC • HESR • Beam lines • Cryogenics • Controls • Civil Engineering • Radiation Safety
Cost OptimizationCivil Construction B3 B1 B2 B14 B7/7a
Cost OptimizationAccelerators • Change of p_bar operation • Repositioning of HESR • Repositioning of FLAIR Cave • Repositioning of PP, AP, CBM caves
FAIR GmbH with international shareholders Company General Assembly International Steering Commitee Scietific / Technical Advisory Committees Administrative Council Supervisory Board Administration and Financial Issues WG Controlling,Legal Issues Safety Scientific Council EU Contracts, 3rd Party Funding Directorate DG Sci. Tech. Admin. FAIR International FAIR Project Management Board Scientific and Technical Issues WG Users, Public Relations FAIR Project Management Team Research Division Infrastructure Division Administration Accelerator Operation FAIR Division (FAIR Technical Director) HADES Buildings Facility Maintenance Central Services Human Resources Injectors Integration ALICE Finance Beam Diagnostics Civil Construction FOPI FRS/ESR HF Accelerator Technical Services Purchasing HE Reactions Theory /systems Operating IT Spectroscopy Rings Experiment Electronics Electrical Engineering Controls SHE / Chemistry SC Magnets Atomic Physics Detector-Lab. HD-Therapy Cryosystems Vacuum PHELIX+PP Target-Lab. Bio Physics FAIR Experiments -TI Documentation / Library CBM -TI Material Research PANDA-TI Theory Super-FRS-TI RIB Low Energy Branch TI CBM RIB High Energy Cave TI PANDA RIB Ring Branch TI TI= Technical Infrastructure NUSTAR Exp. groups FLAIR & SPARC & Applications Facilities TI Plasma Physics TI FLAIR & SPARC
Convention(Governmental Contract –provisions for general framework, procedures, arrangements; annexes?) Articles of Association (based on rules of German limited liability company (GmbH) law; recorded and registered with notary public; any changes require full notary public process) By-Laws (contract(s) on specific rules and regulations between shareholders; does not require notary public involvement) plus additional bi-lateral, multi-lateral contracts, MoU's etc between shareholders and other parties
Cash In-kind: A country delivers a component(e.g., all dipole magnets for one of the rings) Recognized as an equivalent cash contribution Price fixed by STI and its subgroups Cost book for all components Advantage for in-kind takers: Money stays more likely at home Consortia (e.g., HESR consortium, ....): Several partners delivering a component together Form of contributions:
Contract(s) Development Contract(s) Negotiations Closing Evaluation by Advisory Committees by Mid March 05 Cost Review by CORE groups by summer 05 Project Definition in 2005 TDR's The ISC-FAIR International Working Groups AFI Signing of MoU Phase II Governed by Contracts MoU Phase I – Governed by MoU 2005 2004 2006 STI LoI's Proposals / TR's (2100 authors) Technical Committee PAC's
Next Steps 2005 September Consolidated Layout of FAIR October Final Modification of Civil Engineering --> new design specs to BUNG compagny September STI Draft of FAIR definition September/November Cost Review Groups E and A evaluation reports November STI and AFI joint session to finalize FAIR definition November TAC evaluation of new layout, of civil engineering November presentation of project definition to ISC January 2006 Civil Engineering report from BUNG company January 2006 Determination of Legal Structure of FAIR, draft of FAIR contract January-March 2006 TDR - FAIR Project Definition Mid 2006 Signature of FAIR Convention 2006 to 2010 Technical Design Reports (TDR) for the sub systems spring 2008 Start of FAIR construction 2011 – 2014 Commissioning of FAIR
FLAIR@FAIR: Facility for Low energy Antiprotons and Ion Research 100x more intensity than at CERN AD Originates from CERN-AD program “Angels and Demons” at Darmstadt
ISC Decisions The Steering Committee considers the concept proposed for the organisational structure of FAIR as basically appropriate, both for construction and operation. It thus supports: 1. the legal form of a German limited liability company (GmbH), 2. the proposed extension of the present GSI GmbH with international shareholders from the FAIR partner countries and 3. the development of the FAIR convention as well as appropriate articles of association and by-laws, as a basis for the future contractual negotiations and agreements between the partner countries. The signature of the Convention is envisaged for the summer of 2006. For the selection of candidates for the positions of FAIR Project Director and Head of the FAIR Division an international search committee will be set up by the Supervisory Board of GSI.
Mio € year Total cost: 989 Mio € ( Investment cost, additional Personel and including cost escalation )
Organizational Structure of the FAIR Project International FAIR Project Management Board Project Director, Deputy Director Research Coordinator, Accelerator Coordinator, Civil Construction Coordinator, Technical Integration Coordinator, Administrative Coordinator FAIR Project Management Team Contracts & Legal, Budget & Finances, Scientific Coordination, Accelerator Technical Coordination, Civil Construction & Regulatory Procedures, International Project Integration Advisory Committees PACs, TAC, EMAC,... Accelerator Technical Board Research Technical Board Civil Construction Integration Board SIS18 Upgrade 1. P-Linac 2. Acc. System Physics 5. SIS100 3. PANDA 9. CR System 6. Super-FRS 11. SIS200 6T 4. HESR 7. NESR 8. CBM 10. Plasma Phys. Exp. 12. Buildings + Infrastructure 14. Atomic Phys. Exp. 13. Integration 15.
National and International Matters • First Official Public Hearing on FAIR on January 26th, 2005 at GSI • New Consortia in ‘statu nascendi’ and Old ones strengthening: • NESR: Spain- GSI • SIS300: France-Italy-UK- GSI- Russia • Super FRS: GSI-Kolkata • HESR: Jülich-GSI-Uppsala-Stockholm-Novosibirsk-Finland • P-Linac: Frankfurt-ITEP-GSI-India
General strategy: Groundwork, supply systems and major buildings as early as financially possible (potential for smoothing financial profile?) Scientific facilities staged according to three science programmes Contributions from outside mainly in kind for scientific facilities 3-Phase Project Staging
Three stages according to fields of physics: Radioactive beam physics Nuclear structure and nuclear astrophysics Atomic physics studies with highly charged/radioactive ions Proton-antiproton physics QCD studies with protons and antiprotons Precision studies with antiproton beams addressing fundamental symmetries and interactions Full facility research Full parallel operation of up to four experiments Full energy and luminosity for nuclear collisions program at CBM Precision QCD Studies at PANDA up to 8 GeV Plasma research (full gain factor in power density: ~400) Atomic reaction studies with fast beams 3-Phase Project Staging
Civil Construction • Ringtunnel for double ring synchrotron incl. technical buildings • Buildings housing the Super-FRS, 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 Staged construction scenario Stage 1: 2007 - 2010
Civil Construction (completed) • 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 protons and antiprotons • Precision studies with antiprotonn beams addressing fundamental symmetries and interactions Stage 2: 2008 - 2013 HESR
Stage 3: 2010 - 2014 • 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 nuclear collisions 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 experiments