Strategy for the FAIR science program Boris Sharkov Scientific managing director FAIR NuPECC Sweden FranceIndia Finland GermanyPoland Spain Romania Russia Slovenia UK Outline Status and recent news FAIRs full scope confirmed Day-one experimental program Funding status Crucial decisions of international partners regarding scope, cost cap, time line joint Scientific Council FAIR/GSI From MSV to Full Version Beyond the Full Version Boris Sharkov, NuPECC, Jan 20162 NuPECCs Long Range Plan 2010 Unanimous agreement among the European Nuclear Physics community that FAIR shall be one of their top priorities. FAIR would be the largest new Nuclear Physics facilities in Europe, in fact, the world. LRP 2010: Complete in a timely fashion the construction of the Nuclear Physics facilities on the ESFRI list of large-scale research infrastructure projects in Europe: FAIR in DarmstadtPANDA NUSTAR CBM APPA FAIR in Darmstadt, including its four pillars, the PANDA experiment using antiprotons to study the structure and spectroscopy of strongly interacting particles (hadrons), the NUSTAR radioactive beam facility to produce nuclei far from stability and investigate their structure, the CBM experiment to measure the properties of dense baryonic matter, and the atomic, plasma, and applied physics program APPA. 3Boris Sharkov, NuPECC, Jan 2016 Facility for Antiproton and Ion Research FAIR 4 Dense Bulk Plasmas (Ion-beam bunch compression & petawatt-laser) Dense Bulk Plasmas (Ion-beam bunch compression & petawatt-laser) Materials Science & Radiation Biology (Ion & antiproton beams) Materials Science & Radiation Biology (Ion & antiproton beams) Accelerator Physics UNILAC SIS18 SIS100/300p-Linac HESR CR & RESR NESR Cryring Rare-Isotope Production Target Anti-Proton Production Target 100 m QCD-Phase Diagram (HI beams 2 to 45 GeV/u) QCD-Phase Diagram (HI beams 2 to 45 GeV/u) Hadron Physics (Stored and cooled 14 GeV/c anti-protons) Hadron Physics (Stored and cooled 14 GeV/c anti-protons) Nuclear Structure & Astrophysics (Rare-isotope beams) Nuclear Structure & Astrophysics (Rare-isotope beams) Fundamental Symmetries & Ultra-High EM Fields (Antiprotons & highly stripped ions) Fundamental Symmetries & Ultra-High EM Fields (Antiprotons & highly stripped ions) Boris Sharkov, NuPECC, Jan 2016 NuPECC LRP 2010 NuPECCs recommendations were decisive for getting the FAIR-project approved by the governments of the participating European states (including Russia) and beyond (e.g. India) 5Boris Sharkov, NuPECC, Jan 2016 UNILAC SIS18 SIS100/300 p-Linac HESR CR & RESR NESR Cryring Rare-Isotope Production Target Anti-Proton Production Target 100 m Status of the 4 FAIR Experiments Conception of FAIR experiments (Convention) 4 scientific pillars APPA CBM NUSTAR PANDA Experiments funded by 78 M through shares remaining 2/3 by additional funds from shareholders and non-shareholders Boris Sharkov, NuPECC, Jan APPA NUSTAR PANDA CBM/HADES Status of FAIR Experiments Collaborations finalise design and construct components now Boris Sharkov, NuPECC, Jan FAIR Research Division support Technical: Expert Committee Experiments Technical Coordinators Resources: Resources Review Boards Resources Coordinators Computing and simulation: IT Coordinator About 1800 senior scientists (ca in total) members of the FAIR Collaborations Experiments 4 th RRBs and 16 th Council Boris Sharkov, NuPECC, Jan Cost estimate Jan 2015, Collaborations input to 4 th meetings of the Resources Review Boards (RRBs) 245 M (2015 prices) = 196 M (2005 prices) Breakdown (2005 prices) FAIRs part: 78 M in FAIR budget Other approved funding: 35 M Expressions of Interest: 68 M To be assigned: 15 M estimate Status of the FAIR Experiments TDRs submitted and costs covered 9 Covered up to date: 73% Boris Sharkov, NuPECC, Jan 2016 APPA Day-One (examples) Boris Sharkov, NuPECC, Jan BIOMAT (Biophysics and Materials Research) -Materials under extreme conditions (pressure, heat, irradiation) -Radiation shielding of cosmic radiation Day-1 experiments (TDRs: 1 in preparation) Sample irradiation at APPA cave using high pressure cells Irradiation of biological samples at APPA cave HEDgeHOB/WDM (Plasma Physics) -Phase transitions shocked/compressed matter -Opacity measurements of Warm Dense Matter Day-1 experiments (TDRs: 5 approved, 1 submitted, 4 in preparation) Proton microscopy of shocked/compressed materials at APPA cave Opacity changes from Cold- to Warm Dense-Matter at APPA cave SPARC (Atomic Physics) -Precision test of QED in the strong field domain (Z 1) -Model independent determination of nuclear parameter Day-1 experiments (TDRs: 2 approved, 5 submitted, 1 in preparation) Ion channeling at APPA cave Laser spectroscopy at HESR (fine-structure) and at CRYRING (hyperfine) CBM Science at Day-One Boris Sharkov, NuPECC, Jan Observables: Excitation function of yields and phase-space distributions of multi-strange hyperons and lepton pairs in Au+Au collisions from 2-11 A GeV (no data available in this energy range). Physics case Exploring the QCD phase diagram at neutron star core densities CBM Day-One Boris Sharkov, NuPECC, Jan HADES: p+p, p+A, A+A small collision systems CBM: p+A, A+A all collision systems ComponentStatus TDR Dipole Magnetapproved Micro-Vertex Detector2016 Silicon Tracking Systemapproved RICH Detectorapproved TRD (start version)2016 Muon Detector (start version)approved TOF-Detectorapproved Projectile Spectator Detectorapproved DAQ/HPC cluster (start version)2016 HADES Electromagnetic Cal.approved NUSTAR Science at Day-One Boris Sharkov, NuPECC, Jan rd waiting point r-process path GS I Phase-0 Phase-1 Phase-2 NUSTAR aims to measure: -masses --lifetimes -neutron-branchings -strength distributions -level structure Mass abundances depend on the detailed structure of N=126 nuclei around the 3 rd r-process waiting point NUSTAR phases Phase-0: R&D and experiments in existing facilities Phase-1: First measurements with Super-FRS beams Phase-2: Full MSV power One example NUSTAR work packages HISPEC/ DESPEC Boris Sharkov, NuPECC, Jan MATS LaSpec R3BR3B ILIMA TDR approved TDR submitted TDR in preparation No TDR expected LEB/ Super-FRS NUSTAR wps for Day-One experiments HISPEC/ DESPEC Boris Sharkov, NuPECC, Jan MATS LaSpec R3BR3B ILIMA TDR approved TDR submitted TDR in preparation No TDR expected LEB/ Super-FRS Day-1 experiments PANDA Day-One Science Science re-assessed, sharpened and day-one experiments defined Scrutiny Group (reports) EMMI Rapid Reaction Taskforce Physics Workshop Uppsala Key experiments (initial conditions) Scan of narrow resonances X(3872) and newly discovered narrow states and study of radiative decays Formation experiment of Z-resonances using a deuterium target Additional day-one measurements Time-like form factors Excited hyperons Precision charmonium spectroscopy e.g. c1,2 Delta Delta content of Deuteron Requirements: Target, Tracking and Calorimetry Boris Sharkov, NuPECC, Jan PANDA Day-One Technical Status Equipment for day-one experiments Most TDRs approved (covering 71% of full cost of setup) One TDR under review by ECE Three TDRs to be submitted in the upcoming months Two TDRs to profit from IT development 2-3 years before start of operation Further components for future optimised operation Full PID setup Full acceptance/resolution tracking Pellet Target Higher rate DAQ Boris Sharkov, NuPECC, Jan GEM Cluster Solenoid Muon GEM Dipole Muon Range Luminosity Plane Target Detectors Plane System Detector Part Barrel DIRC MVD STT Barrel FE Part FToF FSC EMC EMC F-Trk BE EMC PANDA Start Setup 18Boris Sharkov, NuPECC, Jan 2016 GEM & PelletTracker Cluster Solenoid Muon GEM Dipole Muon Range Luminosity & Pellet Detectors Tracker System Detector Target DiscFullFRICH Barrel DIRC MVD STT Barrel Disc FE Full FRICH FToF FSC Barrel ToFDIRC Barrel ToF EMC DIRC EMC F-Trk BE EMC PANDA Final Setup Boris Sharkov, NuPECC, Jan Current Status of the FAIR-Experiments All four FAIR Collaborations have re-assessed their experimental programme and instrumentation in view of Progress in science, the changed timeline and availability of funding The programme for day-one experiments starting in 2022 has been developed Prioritising for max. scientific merit and concentrating on the initially required equipment 20Boris Sharkov, NuPECC, Jan 2016 The Modularised Start Version (MSV) 21 APPA CBM/HADES NUSTAR PANDA Modules M0: SIS100 M1: APPA M1: CBM/HADES M2: NUSTAR M3: PANDA, NuSTAR, APPA M0 M1 M2 M3 Cost about 1.6 billion by 2018 (1 billion 2005 Euros) Boris Sharkov, NuPECC, Jan 2016 Observations and Recommendations by SC as of The Scientific Councils (SCs) reconfirm their earlier assessment that all four FAIR pillars - despite the delay of the project - carry compelling scientific cases with unique discovery potential. 2.Therefore, the SCs consider the FAIR MSV to offer the best science to cost ratio for the FAIR project. 3.The SCs carefully took into account the recommendations by the International Review Committee chaired by Rolf Heuer. The SCs consider the ordering of the experiments as the result of a resource-loaded rather than a purely scientific evaluation. Boris Sharkov, NuPECC, Jan Council Decision, Sept 2015 The Council agrees to the immediate merger of the FAIR Scientific Council and the GSI Scientific Council. Nuclear Physics (3) Bob Tribble (BNL, USA) Maria J.G. Borge (Madrid, Spain) Faial Azaiez (IPN Orsay, France) Atomic & Laser Physics (3) Eva Lindroth (Stockholm, Sweden) Lembit Sihver (Vienna, Austria; also med.rad. phys) Klaus Blaum (MPIK Heidelberg, Germany) Heavy Ion / Compressed Matter (3) Sibaji Raha (Kolkata, India) Krzysztof Redlich (Wroclaw, Poland) Christelle Roy (CNRS Strasbourg, France) Hadron Physics (2) Patrizia Rossi (JLab, USA) Naohito Saito (J-PARC, Japan) Accelerator / Rings (1) Grigory Trubnikov (JINR, Russia) Boris Sharkov, NuPECC, Jan Council Decisions Boris Sharkov, NuPECC, Jan Decision XVII.6.1 (1)The Council confirms the stepwise approach to the realization of the FAIR project outlined in the Convention, Article 5 (6), starting with the Modularized Start Version (MSV), according to Article 5 (2) of the Convention. (2) The Council states that the target completion date for the Modularized Start Version should be not later than (3) The Council asks the FAIR Management to provide for approval by the Council a suitable document summarizing the reasons for the delay in realization of FAIR and the respective cost increases as well as a reasoned proposal of the MSV construction time scale and financing schedule, in a manner which is communicable to decision makers in all partner countries. (4) Taking into account the prolonged time schedule for the realization of the FAIR Modularized Start Version and the concomitant cost increases, a staged approach is agreed upon for speeding up the start of experiments. (5) The Council asks the Management to prepare for a detailed review of the progress and financial status of the FAIR project not later than 2019. High Level Schedule of the MSV Boris Sharkov, NuPECC, Jan Costs of the MSV for the FAIR-Shareholders Boris Sharkov, NuPECC, Jan Total costs (M)2005 pricesEscalated prices* Experiments Accelerators Acc. coordination personnel Personnel FAIR GmbH Running costs Civil Construction original estimate 78,0 385,0 110,9 38,0 15,4 495,0 83,6 412,5 113,1 43,1 19,8 676,3 Subtotal1.122,31.348,4 less site costs1.027,31.220,9 Civil Construction cost increase227,9 320,1 LEB buildingLEB building6,59,6 Total incl. site costs1.356,81.678,1 Costs for setting up the experiments as allocated in the FAIR-budget Higher costs of civil construction (320 million , as escalated to the finishing date) not yet covered Council Decisions II Boris Sharkov, NuPECC, Jan cost cap (6) The Council defines the value of 1,262 M (2005 prices) as cost cap for the FAIR Modularized Start Version, not including the exceptional additional site-related costs of 95 M (2005 prices), already borne by Germany. (7) In order to enable the Management to expedite contracting of design works, civil construction, and accelerator and detector component construction for all four FAIR experimental areas in the framework of the MSV, the Council asks the Shareholders and the Associated Partner to assure the necessary additional funding as soon as possible (cf. Table 1). Commitments to cover additional 158 M (2005 prices) have to be made at the latest by the end of the first half of 2016; commitments to cover another 90 M (2005 prices) will have to be made by This additional funding will be required from 2019 onwards for the completion of the MSV, and is to be provided in principle as cash contribution. (8) The Council asks the Management to continuously look for any cost saving measures. (9) The Council asks the Management to continue its effort to attract additional Shareholders to the project who will be able to bring in additional intellectual and financial resources for the project. Conclusions Despite of certain delays FAIR is progressing well. Rich scientific program and discovery potential already with completion of Modularized Start Version. FAIR will allow for unique measurements in many fields and remain competitive for decades. Versatile detector configurations for optimal performance are under construction. Day-one physics case with start version for high interaction rates in preparation. Strong and experienced international collaborations are active, more scientists expected to join in the coming years. 28Boris Sharkov, NuPECC, Jan 2016 From MSV to Full Version of FAIR Boris Sharkov, NuPECC, Jan UNILAC SIS18 SIS100/300 p-Linac HESR CR & RESR NESR Cryring Rare-Isotope Production Target Anti-Proton Production Target 100 m Blue: existing Red: to be built within MSV Yellow: beyond MSV Boris Sharkov, NuPECC, Jan Staging Plan ( ) Baseline Technical Report 2005 Start Version Phase A 2007 (SIS100) Phase B (SIS300) Modularised Start Version 2009 Module 0Module 1Module 2Module 3Module 4Module 5 SIS100Exp. halls CBM & APPA Super-FRS NuSTAR Antiproton Facility PANDA & options NuSTAR LEB, NESR, FLAIR NuSTAR & APPA RESR PANDA, NuSTAR & APPA Based on recent cost estimates (2009) and the funding commitments of the FAIR Member States MSV of the Projects comprises modules 0 3. Good News LEB building again on board that means: MATS/LaSpec, HISPEC/DESPEC, debuncher... to be installed as planned SIS100 / SIS300 tunnel design not changed that means: SIS300 (beyond MSV) can be installed without major modifications 31Boris Sharkov, NuPECC, Jan 2016 NUSTAR Experimental areas 32 Production target ILIMA R3BR3B HISPEC/DESPEC MATS & LaSpec Super-FRS Boris Sharkov, NuPECC, Jan 2016 NUSTAR The Project Super- FRS RIB production, separation, and identification Super- FRS exp. collabor. High-resolution spectrometer experiments HISPEC/ DESPEC In-beam -spectroscopy at low and intermediate energy, n-decay, high-resolution -, -, -, p-, spectroscopy MATS/ LaSpec In-trap mass measurements and decay studies + Laser spectroscopy R3BR3B Kinematical complete reactions with relativistic radioactive beams ILIMA Large-scale scans of mass and lifetimes of nuclei in ground and isomeric states EXLLight-ion scattering reactions in inverse kinematics SHESynthesis and study of super-heavy elements ELISeElastic, inelastic, and quasi-free e - -A scattering 33 The Collaboration > 800 scientists > 180 institutes 38 countries The Collaboration > 800 scientists > 180 institutes 38 countries The Investment 82 M Super-FRS 73 M Experiments The Investment 82 M Super-FRS 73 M Experiments The Approach Complementary measurements leading to consistent answers The Approach Complementary measurements leading to consistent answers Boris Sharkov, NuPECC, Jan 2016 Midterm Strategy beyond MSV Reach full power of FAIR (at the earliest possible) Installation of RESR Full luminosity antiproton program with PANDA Enable parallel operation Installation of SIS300 Stretching mode for NUSTAR experiments High energy (up to 35 GeV/u /s 238 U 73+ ) for CBM Parallel operation of up to 6 experiments Enable FLAIR, (SPARC), EXL, ELISe science Consider options for cost-effective up-to-date solutions (e.g. using connection beam lines HESR-ESR-CRYRING) Details to be refined closer to the finalisation of MSV 34Boris Sharkov, NuPECC, Jan 2016 SIS18 - HESR Connection Options for FAIR beyond MSV 35 (4) pbar-Target Bypass SIS18 -> CR (13 Tm) In MSV (1) HESR West Injection SIS18 -> HESR (13 Tm) Beyond MSV (2) HESR North East Extraction HESR -> ESR (7 Tm) Beyond MSV (3) HESR North East Injection SIS18 -> HESR (7 Tm or 13 Tm) Beyond MSV Figure taken from Preliminary Report HESR-Beamlines Karl-Heinz Kampert, Jaques Martino October E. Mahner Boris Sharkov, NuPECC, Jan 2016 Long-Term Strategy Optimise the strategy as outlined in NuPECCs 2010 LRP LRP 2010 polarised Electron-Nucleon Collider (ENC) at FAIR Polarised Antiproton eXperiments (PAX) at FAIR Organise dedicated workshop(s) under NuPECCs umbrella Investigate discovery potential and competiveness Technical feasibility and required resources Funding Boris Sharkov, NuPECC, Jan NuPECCs LRPs NuPECCs recommendations were decisive for getting the project approved by the governments of the participating European states and beyond and will be decisive for the future development of the FAIR international research centre at Darmstadt towards the full FAIR version and beyond 37Boris Sharkov, NuPECC, Jan 2016 Thank you very much Boris Sharkov, NuPECC, Jan 39 The scientific goals of the ENC comprise the precise determination of the spin flavour structure of the nucleon consisting of quarks and gluons. The science case has to be evaluated in view of the Electron Ion Colliders (EIC) scientific reach and progress. (EIC planned at Brookhaven or JLab) NuPECC LRP 2010: ENC at FAIR Boris Sharkov, NuPECC, Jan 2016 40 Proposed accelerator layout to convert the HESR into a double-polarised proton-antiproton collider. Polarised antiprotons are produced in the Antiproton Polariser Ring (APR) and then injected in the (COSY-like) Cooler Synchrotron Ring (CSR). Polarised protons will circulate in the HESR. NuPECC LRP 2010: PAX at FAIR Boris Sharkov, NuPECC, Jan 2016 Successful tests and preparations at COSY Pending tests with longitudinal polarisation and antiprotons