Status of the FAIR Project I Augustin FAIR

Status of the FAIR Project I. Augustin FAIR Coordination Group GSI September 19, 2006 I. Augustin, GSI at PHIBADE 2006

CDR Layout at pre-FAIR times 2001 700 authors PANDA Plasma Phys. Low En. RIB Expt. High En. RIB Expt. CBM Atom. Phys. September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

International FAIR Project: the Intensity Frontier Primary Beams Key Technologies • All elements up to Uranium • Factor 100 -1000 over present intensity • 50 ns bunching • Beam cooling • Rapidly cycling superconducting magnets • Narrow bunching of beams Secondary Beams Rare Isotope Production Target • Rare isotope beams up to a factor of 10 000 in intensity over present • Low and high energy antiprotons Antiproton Production Target September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg Storage and Cooler Rings • Rare isotope beams • e-– Rare Isotope collider • 1011 stored and cooled antiprotons for Antimatter creation

Radioactive Ion Beam Programme Plasma Physics Beam Programme September 19, 2006 Anti Proton Beam Programme Relat. Ion Beam Programme I. Augustin, GSI at PHIBADE 2006, Strasbourg

Up to 4 fold Parallel Operation at FAIR ! September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

The International Committee Structure of FAIR ISC International Steering Committee H. Schunck STI Working Group AFI Working Group Scientific + Technical Issues Administrative + Funding Issues H. Wenninger / S. Gales Ö. Skeppstedt PAC QCD E. Chiavassa FAIR Project Legal Framework Issues PAC NUSTAR R. Casten U. B. Jahn FCI PAC APPA D. Schwalm TAC Y. Cho CORE Cost Review Groups Full Cost Issues Mini. TACs • Cryogenics • Warm and Cold magnets • Power Supplies • Beam Instrumentation • p-Linac D. Plane, W. Bartel Observers: September 19, 2006 LFI I. Augustin, GSI at PHIBADE 2006, Strasbourg B. Brandt

Milestones 2003 – 2006 September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

Baseline Technical Report (April 2006) > 3500 pages Contributors: ~ 2200 expt. scientists ~ 400 accel. scientists Investment costs: ~ 1000 M€ Personnel needed: ~ 2400 MY September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

FAIR LAYOUT September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

What has changed? • readjusting of the beam rigidity (SIS 300) • optimizations injection and extraction of the synchrotrons • rearrangement high energy beam transport system • add storage ring (RESR) to achieve the accumulation and cooling performance • antiproton injection into HESR at an energy of 3 Ge. V • accelerate/decelerate in HESR allowing direct injection from RESR September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

FLAIR@FAIR: Facility for Low energy Antiprotons and Ion Research 100 x more intensity than at CERN AD Originates from CERN-AD program September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

STI Recommendations on Experiments Experiment PAC Base Program Core Facility R 3 B NUSTAR yes HISPEC/DESPEC NUSTAR yes ILIMA NUSTAR yes LASPEC NUSTAR yes MATS NUSTAR yes AIC NUSTAR no no ELISe NUSTAR yes EXL NUSTAR yes NCAP NUSTAR no no EXO-pbar NUSTAR no no PANDA QCD yes CBM QCD yes PAX QCD no no Strong scientific merit; could become part of base program ASSIA QCD no no Consider joining PAX LAPLACE/HIHEX/WDM APPA yes should merge under one umbrella FLAIR APPA no yes not part of the initial CDR SPARC APPA yes BIOMAT APPA yes September 19, 2006 Comments open scientific & techn. issues request beam-time I. Augustin, GSI at PHIBADE 2006, Strasbourg

Accelerator Physics and Technology for FAIR Main 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 Fast stochastic and electron cooling HESR e-cooler September 19, 2006 Ultra high vacuum for intense beams Control of collective effects: Large scale simulation studies Desorption test-stand I. Augustin, GSI at PHIBADE 2006, Strasbourg Working point diagram: Stability of intense beams

Critical Path Issues Negotiations and agreements with FAIR partners: • • • Decisions on NESR, RESR magnet technology (warm or cold) in autumn of 2006 Spain If decision for NESR and RESR superconducting, prototype for end of 2008 Spain CR and Super FRS sc-dipole prototypes in 2008 China SIS 300 decision for or against curved magnets probably end of 2006 Italy, Russia SIS 300 sc magnets prototype a) straight magnets 2008, b) curved magnets 2008/9 Italy, Russia SIS 300 sc quadrupoles prototype 2008/9 France, CEA and IN 2 P 3 SIS 100 sc magnet prototype 2008 Russia, Industry, GSI HESR curved sc magnets, feasibility study end 2006, prototype in 2008 Industry, Jülich Design Super FRS Triplets 2007 Industry, GSI Prototype Super FRS Triplet 2008 Industry, GSI SUPER FRS Energy Buncher dipoles, delivery end of 2009 India September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

R&D funding issues: FAIR - EU support EU R&D funding FAIR related amounts to 32 M€ SIS 100/SIS 300 SIS 18 HADES* / CBM I 3 HP GSI Accelerator Facilities R 3 B HADES* HESR Super- FRS PANDA (I 3 HP) R 3 B CR NESR NUSTAR EURONS Scope of CNI: FAIR injector SIS 18 intensity upgrade (HADES, R 3 B) Scope of Design Study: secondary beams (RIB and Antiprotons) I 3 programmes in the 6 th FP I 3 HP, EURONS, September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

FAIR Master Schedule Adapted to Civil Construction Schedule Critical Path: Availability of buildings to start installations (Subjected for further optimization) Actual planning allows for: Ø First experiments at s. FRS 2011/2012 Ø Project end 2014/2015 September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

Stage 1 (2007 - 2011) Radioactive beam physics • Nuclear structure and nuclear astrophysics • Atomic physics studies with highly charged/radioactive ions & plasma physics Civil Construction Activity September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

Stage 2 (2011 - 2013) Proton-antiproton physics • QCD studies with protons and antiprotons • Precision studies with antiproton beams addressing fundamental symmetries and interactions • FLAIR Relat. Heavy Ions • 1 -10 AGe. V relat. heavy ion beams for atomic and nuclear collision studies, e. g. with HADES Civil Construction Activity September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

Stage 3 (2013 - 2015) Full facility capability & all research programs No Civil Construction Activity anymore September 19, 2006 • 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 Ge. V/c • Plasma research (full gain factor in power density: ~400) • Atomic reaction studies with fast beams I. Augustin, GSI at PHIBADE 2006, Strasbourg

Proposed FAIR – Roadmap: Establishment of FAIR Gmb. H meetings ISC 07/06 Contracting Parties STI AFI 08 ISC 09 10 11 Negotiations (ongoing, 'till end of 2006) 12 01/07 Nomination of Shareholders + Completion of negotiations AFI STI Bylaw Subgroup Mandate for IKAB 03 04 05 Signature Formation Constitutive Ao. A FAIR Gmb. H Meeting of the Council Convention, Bylaws, draft FAIR Final Act, Ao. A; Gmb. H structure and Joint Core Team kick-off staffing Elaboration of the Bylaws (ongoing) Completion of draft Bylaws Technical project decisions (follow up design changes) / FAIR preparation tasks (ongoing process up to the foundation of FAIR Gmb. H) Technical evaluation of potential in-kind contributions (ongoing process up to the formation of FAIR Gmb. H) September 19, 2006 06 Signature of Convention and Final Act Convention, Bylaws, draft FAIR Final Act, Ao. A; structure Bylaws (first draft) Monitoring of technical planning and project costs (ongoing process up to the formation of FAIR Gmb. H) Joint Core. Team IKAB 02 First meeting: start senior staffing Shareholders (SH) ISC Convention Final Act Ao. A joint meeting ISC/SH AFI I. Augustin, GSI at PHIBADE 2006

Thank you for your attention! September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

Parameters for end of commissioning / start of operation (I) September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

Parameters for end of commissioning / start of operation (II) September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

There are other IN-FLIGHT and ISOL facilities availabe WHY FAIR ? The FAIR accelerators will provide beams with the following characteristics: Full range of ion beam species plus antiprotons: The facility will accelerate all ions from protons (and also antiprotons) up to heaviest elements, uranium. This will provide the necessary broad basis for the multi-disciplinary research program for FAIR. Highest beam intensities: Intensities of primary heavy-ion beams will increase by a factor of 100, secondary radioactive beams by a factor of up to 10, 000 over the present GSI facility, pushing forwards the sensitivity of experiments Substantial increase in beam energy: An increase by about a factor of 20 in energy is foreseen for beams as heavy as uranium. In this energy regime nucleus-nucleus collisions are expected to generate hadronic matter at the highest densities This enables unique studies of charm production in highly compressed matter. Generation of precision beams: These will be stochastic and electron cooling of ion beams, in particular also applicable to the secondary radioactive and antiproton beams. Together with the statistical precision and high sensitivity that results from high beam intensities and interaction rates, the precision-quality beams will allow entering totally new areas of research in all of the FAIR science fields. Synchrotrons and storage rings as accelerator structures of choice: For ion beams, ranging from protons to uranium, synchrotrons provide the most economical solution to generate very high beam energies. Even more important for the FAIR research program, accelerator rings are unique in their capability to store, cool, bunch, and stretch beams. September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

Five Research Communities at FAIR SIS 100/300 CBM HADES HESR Rare Isotope Production Target Hadron Physics with antiprotons of 0 - 15 Ge. V Plasma Physics: x 600 higher target energy density 600 k. J/g Nuclear Matter Physics with 35 -45 Ge. V/u HI beams, x 1000 Super FRS FLAIR CRRESR Antiproton Production Target Nuclear Structure & Astrophysics with radioactive beams, x 10 000 and excellent cooling NESR 100 m September 19, 2006 High EM Field (HI) _ Fundamental Studies (HI & p) Applications (HI) I. Augustin, GSI at PHIBADE 2006, Strasbourg