September 19, 2006
- I. Augustin, GSI at PHIBADE 2006
Status of the FAIR Project Status of the FAIR Project
- I. Augustin
Status of the FAIR Project Status of the FAIR Project I. Augustin - - PowerPoint PPT Presentation
Status of the FAIR Project 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 Low En. RIB Expt. Plasma Phys. High
September 19, 2006
PANDA Atom.Phys. CBM Plasma Phys. Low En. RIB Expt. High En. RIB Expt.
September 19, 2006
September 19, 2006
Primary Beams
intensity
Secondary Beams
factor of 10 000 in intensity
antiprotons
Key Technologies Storage and Cooler Rings
antiprotons for Antimatter creation Rare Isotope Production Target Antiproton Production Target
Radioactive Ion Beam Programme Anti Proton Beam Programme Plasma Physics Beam Programme
September 19, 2006
September 19, 2006
September 19, 2006
PAC QCD E. Chiavassa PAC NUSTAR R. Casten PAC APPA D. Schwalm TAC Y. Cho
Observers:
CORE
Cost Review Groups
FCI
Full Cost Issues
AFI Working Group
Administrative + Funding Issues
Ö. Skeppstedt
LFI
Legal Framework Issues
U.B. Jahn
STI Working Group
Scientific + Technical Issues
International Steering Committee
MiniTACs
September 19, 2006
> 3500 pages Contributors: ~ 2200 expt. scientists ~ 400 accel. scientists Investment costs: ~ 1000 M€ Personnel needed: ~ 2400 MY
September 19, 2006
September 19, 2006
September 19, 2006
September 19, 2006
Originates from CERN-AD program
100x more intensity than at CERN AD
Experiment PAC Base Program Core Facility Comments
R3B NUSTAR yes yes HISPEC/DESPEC NUSTAR yes yes ILIMA NUSTAR yes yes LASPEC NUSTAR yes yes MATS NUSTAR yes yes AIC NUSTAR no no
ELISe NUSTAR yes yes EXL NUSTAR yes yes NCAP NUSTAR no no request beam-time EXO-pbar NUSTAR no no PANDA QCD yes yes CBM QCD yes 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 yes should merge under one umbrella FLAIR APPA no yes not part of the initial CDR SPARC APPA yes yes BIOMAT APPA yes yes
September 19, 2006
Main R&D challenges Main R&D challenges
Novel lattice/collimation design: Beam optics studies High gradient, low frequency RF cavities Superconducting, fast ramping synchrotron magnets
control of stripping losses SIS 100 dipole magnet CR compressor cavity September 19, 2006
Control of collective effects: Large scale simulation studies Ultra high vacuum for intense beams Fast stochastic and electron cooling
Working point diagram: Stability
beams Desorption test-stand HESR e-cooler
Negotiations and agreements with FAIR partners:
Spain
Spain
China
Italy, Russia
Italy, Russia
France, CEA and IN2P3
Russia, Industry, GSI
Industry, Jülich
Industry, GSI
Industry, GSI
India September 19, 2006
Scope of CNI: FAIR injector SIS18 intensity upgrade (HADES, R3B) Scope of Design Study: secondary beams (RIB and Antiprotons) I3 programmes in the 6th FP I3HP, EURONS,
SIS100/SIS300
HESR
PANDA (I3HP)
CR
GSI Accelerator Facilities
NESR
Super- FRS
HADES* / CBM I3HP NUSTAR EURONS HADES* R3B R3B
SIS18
EU R&D funding FAIR related amounts to 32 M€
September 19, 2006
September 19, 2006
FAIR Master Schedule
Adapted to Civil Construction Schedule Critical Path: Availability of buildings to start installations (Subjected for further optimization) Actual planning allows for:
First experiments at sFRS 2011/2012 Project end 2014/2015
September 19, 2006
(2007- 2011)
Civil Construction Activity
nuclear astrophysics
studies with highly charged/radioactive ions & plasma physics
September 19, 2006
(2011- 2013)
Civil Construction Activity
Proton-antiproton physics
and antiprotons
antiproton beams addressing fundamental symmetries and interactions
beams for atomic and nuclear collision studies, e.g. with HADES
September 19, 2006
(2013- 2015)
No Civil Construction Activity anymore
four research programs
nuclear collisions program at CBM
PANDA up to 15 GeV/c
in power density: ~400)
fast beams
September 19, 2006
Proposed FAIR – Roadmap: Establishment of FAIR GmbH
07/06 08 09 10 11 12 01/07 02 03 04 05 06 Nomination of Shareholders + Completion
Completion
Bylaws Signature of Convention and Final Act Signature AoA
STI AFI AFI joint meeting ISC/SH ISC ISC
Bylaws, draft FAIR GmbH structure and kick-off staffing Convention, Final Act, AoA; Joint Core Team Technical evaluation of potential in-kind contributions (ongoing process up to the formation of FAIR GmbH) Mandate for IKAB Monitoring of technical planning and project costs (ongoing process up to the formation of FAIR GmbH) Elaboration of the Bylaws (ongoing) Convention Final Act
AoA
First meeting: start senior staffing Constitutive Meeting of the Council Convention, Final Act, AoA; Bylaws (first draft) Bylaws, draft FAIR structure Technical project decisions (follow up design changes) / FAIR preparation tasks (ongoing process up to the foundation of FAIR GmbH) Formation FAIR GmbH Negotiations (ongoing, 'till end of 2006)
meetings
Contracting Parties Share- holders (SH) ISC AFI STI Bylaw Subgroup Joint Core- Team IKAB
September 19, 2006
September 19, 2006
September 19, 2006
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
100 m
High EM Field (HI) _ Fundamental Studies (HI & p) Applications (HI) Plasma Physics: x600 higher target energy density 600kJ/g Nuclear Matter Physics with 35-45 GeV/u HI beams, x1000 Hadron Physics with antiprotons
SIS 100/300
HESR Super FRS NESR CBM HADES FLAIR CR- RESR
Rare Isotope Production Target Antiproton Production Target
Nuclear Structure & Astrophysics with radioactive beams, x10 000 and excellent cooling
September 19, 2006