FAIR Project in Progress. Boris Sharkov. Scientific managing director. Moscow

Transcription

1 FAIR Project in Progress Boris Sharkov Scientific managing director Moscow Finland France Germany India Poland Romania Russia Slovenia Spain Sweden UK

2 Facility for Antiproton and Ion Research new international research laboratory under construction to explore the nature and evolution of matter in the Universe p-linac SIS18 SIS100/300 UNILAC HESR Rare-Isotope Production Target Anti-Proton Production Target CR & RESR Cryring 100 m NESR 2

3 The FAIR Project 3

4 Accelerator Facility Primary Beams /s; 1.5 GeV/u; 238 U /s 238 U 73+ up to 35 GeV/u 3x10 13 /s 30 GeV protons UNILAC p-linac SIS18 SIS100/300 Secondary Beams range of radioactive beams up to GeV/u; up to factor higher in intensity than presently antiprotons 3-30 GeV Storage and Cooler Rings HESR Rare-Isotope Production Target Anti-Proton Production Target radioactive beams antiprotons GeV/c, stored and cooled Technical Challenges CR & RESR 100 m NESR Cryring cooled beams, rapid cycling superconducting magnets 4

5 Acc Performance for FAIR Experiments Beam Intensities: intensities of primary beams: x 100 x 1000 intensities of secondary beams: x Beam Energies: energies: x 30 Unprecedented Variety of Ions: antiprotons protons to Uranium, radioactive beams Beam Quality: cooled antiprotons intense cooled RIBs Pulse Structure: extremely short pulses (70 ns) to slow extraction (quasi CW) Parallel Operation: (Finally) operation of up to four experiments simultaneously

6 Physics at FAIR Nuclear Structure & Astrophysics (Rare-isotope beams) Hadron Physics (Stored and cooled 14 GeV/c anti-protons) UNILAC p-linac SIS18 SIS100/300 QCD-Phase Diagram (HI beams 2 to 45 GeV/u) Fundamental Symmetries & Ultra-High EM Fields (Antiprotons & highly stripped ions) HESR Rare-Isotope Production Target Anti-Proton Production Target Dense Bulk Plasmas (Ion-beam bunch compression & petawatt-laser) CR & RESR Cryring Materials Science & Radiation Biology (Ion & antiproton beams) 100 m NESR Accelerator Physics 6

7 The 4 Scientific Pillars of FAIR APPA: Atomic, Plasma Physics and Applications CBM: Compressed Baryonic Matter NUSTAR: Nuclear Structure, Astrophysics and Reactions PANDA: Antiproton Annihilations at Darmstadt In total: Users 7

8 Collaboration Members by Country Inti Lehmann FAIR, 95th ECFA, 25/7/2014 8

9 FAIR Members Contributions All numbers in 2005 escalation until 2018 ca. +50% i.e. about 1.6 billion Most contributions in-kind Discussions with Spain and Italy on-going Interested parties ESA, Saudi Arabia, Netherlands, China, Turkey, Brazil, Ukraine, S Korea, Japan, USA 9

10 FAIR Modularised Start Version M3 M0 Science with the MSV M1 M3 M2 CBM Experiments M0: SIS100 M1: CBM,APPA M2: NUSTAR M3: PANDA, APPA, NUSTAR PANDA APPA NUSTAR The MSV should enable realization of outstanding forefront research program to all 4 scientific pillars of FAIR 12

11 FAIR: an international endeavour The FAIR Convention: contractual foundation of FAIR International convention concerning the construction and operation The FAIR company and the GSI will collaborate in the construction, commissioning and operation on the basis of long-term agreements. International partners provide an interest about 30 % Contributions to the construction costs may be provided in-kind or in-cash Shares are costbook based Partners Germany, Russia, Finland, France, India, Poland, Romania, Sweden, Slowenia, United Kingdom 15

12 FAIR: Facility for Antiproton and Ion Research Linked to the existing facility GSI (Darmstadt, Germany) Based upon an international convention New research possibilites with high intensity antiproton and ion beams Stepwise approach to the realisation (Modularized Start Version MSV- modules 0-3.) modules 4 to 6 are scientifically highly desirable MSV provides for outstanding and world-leading research programmes in all four scientific areas: Nuclear, Hadron (Particle), Atomic- and Plasma Physics, Biomedicine and Materials Science Various physics programs can be operated in parallel FAIR will offer outstanding research opportunities for about 3000 scientists from about 50 countries. 17

13 Funds are Rolling In Grants by BMBF/Germany/: 526 M euro for civil construction 65 M euro for the construction of the HESR 53 M euro for the operation of the FAIR GmbH > 40 M euro EU funding 2 July 2012 ~ 100 M euro cash from international partners Permits: General construction permit for all buildings by city of Darmstadt 13 radioprotection licenses received. B. Sharkov 19

14 Accelerator s Status Progressing well SIS 100 dipoles First series del.+tested SIS 100 sextopoles Dubna prototype HEBT magnets Efremov, St Petersburg SIS 100 quadrupoles JINR, Dubna 21

15 Russian Hightech for FAIR IHEP-Protvino JINR Dubna BINP Novosibirsk

16 FAIR + JINR :Searching for nuclear matter at extreme states NICA/MPD Nuclotron-based Ion Collider facility FAIR/CBM E lab < 60 GeV/n snn = GeV/n Average luminosity sm -2 s -1 Au x Au E lab ~ 34 GeV/n snn = 8.5 GeV Particle intensity (for U) up to ppp

17 Cryomagnetic Quadrupole Modules for SIS100 Manufacturing design of first of series module, completed by GSI design department Design service contract for overall cryomagnetic quadrupole module system signed and progressing In-kind & R&D contract for production and testing of quadrupole units with JINR under preparation Manufacturing documents delivered to JINR Production of FoS unis until end of 2015 Design of FoS modul and components by GSI Design Office SIS100 Design of QM module including end boxes (link to local cryogenics) 24

18 The workshop starts magnet production in Dec cable machine has been put in operation workshop is ready for coil production the I-st arm has been put in operation 28 Aug SC magnets for NICA & SIS-100 Fair 15 September 2014 V.Kekelidze, XXII IBSHEPP, Dubna 25

19 FAIR Collector Ring Transfer of CR Project Responsibility to BINP Novosibirsk BINP, FAIR, and GSI are considering the entire CR machine, except the stochastic cooling and RF systems, as Russian contribution. MoU signed during a first visit in Novosibirsk (October). Technical Addendum of MoU discussed and signed during a Workshop in Darmstadt (November) Betriebsversammlung O.

20 In-kind contributions for FAIR Institut Preise in М (Kosten 2005) Experimente Maschine Total Budker INP 4,371 39,404 79, IHEP 13,426 39, JINR 14,933 7,133 33, ITEP 5,123 1,000 28, Efremov NIIEFA 18,795 22, PNPI 8,957 12, Ioffe PTI 0,837 2, IPCP RAS 1,770 1, INR 0,961 1, Kurchatov Institut 2,500 1, MPEI 0,350 0, LPI RAS 0,350 0, CASH ROSATOM 13,640 TOTAL 53,578 79, ,550 27

21 Civil Construction Synchrotrons: 1.1 km HESR: 0.6 km With beamlines: 3.2 km Existing SIS 18 Total area > m 2 Area buildings ~ m 2 Usable area ~ m 2 Volume of buildings ~ m 3 Substructure:~ 1500 pillars, up to 65 m deep 30

22 HEBT (High Energy Beam Transfer) pbar, APPA The High Five (Dallas) SFRS SIS18 CBM SIS100/300 SIS100/300 Batch 1 > 51 dipoles, vacuum chambers Batch 2 > 17 dipoles, 102 quadrupoles, 80 steering magnets, vacuum chambers Batch 3 > 5 dipoles, 71 quadrupoles, 12 steering magnets, vacuum chambers Suppliers > BINP (magnets) and Efremov Institute (vacuum chambers) E. Mahner 31

23 Satellite s View 2.5 km Google Earth for FAIR FAIR AFC 10, Darmstadt, 21/5/14 33

24 Bird s View 34

25 FAIR Construction Site 35

26 Experiments CBM APPA Super- FRS PANDA NuSTAR 36

27 FAIR Collaborations Scientific Councils, Neuenahr, 21/1/14 37

28 Research Division Optimization of integrated timelines in progress Coordination with Accelerators and Civil Construction Early installation of experiments Day 1 experiments (SC + WR) Fully included into Risk Management Construction MoUs to be agreed upon in RRBs Technical Design Reports and their current status Collaboration Approved Submitted Still outstanding Announced for 2014 Total expected APPA CBM NUSTAR PANDA Total B. Sharkov 38

29 Atomic Physics, Plasma Physics, and Applied Sciences Highest Charge States Extreme Static Fields Relativistic Energies Extreme Dynamical Fields and Ultrashort Pulses High Intensities Very High Energy Densities and Pressures High Charge at Low Velocity Large Energy Deposition Low-Energy Anti-Protons Antimatter Research Atomic Physics Plasma Materials Bio SPARC FLAIR HEDgeHOB/WDM MAT/BIOMAT BIO/BIOMAT anti-matter planetary interiors... states of matter strong field research... probing of fundamental laws of physics... matter / antimatter asymmetry common in Jim Ritman astrophysical objects extreme conditions... radiation hardness and modification of materials aerospace engineering... radiation shielding of cosmic radiation

30 The APPA Experimental Facilities ESR Cold Highto Low- + CRYRING Energy Heavy Ions HESR Later Anti-Protons Cold Relativistic Heavy Ions APPA Cave Jim Ritman

31 Route to a consolidated schedule Accelerators Construction Experiments 42

32 Next steps and mission critical issues Number of processes running in parallel disturbed planning process, additional costs for CC, changes in top management, merger Civil construction is presently the lead process. Strengthening of the project governing system + TMD + D S&B Consolidated, synchronized timeline (with CC start a.s.a.p. and the end by the end of the decade) is under elaboration. B. Sharkov 44

33 Outlook I Negotiation of international partners with national authorities on sharing the additional costs for CC. Our asset strong an experienced research community. (Worms 2014). 45

34 The FAIR Project Thank you very much! 46