research areas at fair
DESCRIPTION
Magnetic Fusion. Inertial Cofinement Fusion. Sun Core. Temperature [eV]. PHELIX. Laser Heating. Ideal plasmas. Strongly coupled plasmas. Ion Beam Heating. Jupiter. SIS 18. solid state density. Sun Surface. Density [cm -3 ]. Research Areas at FAIR. - PowerPoint PPT PresentationTRANSCRIPT
Gottfried Münzenberg , FINUPHY, Madeira 2005
Status of FAIR andHeavy and Superheavy Elements
Research Areas at FAIR
Structure and Dynamics of Nuclei - Radioactive BeamsNucleonic matterNuclear astrophysicsFundamental symmetries
Hadron Structure and Quark-Gluon Dynamics - AntiprotonsNon-pertubative QCDQuark-gluon degrees of freedomConfinement and chiral symmetry
Nuclear Matter and the Quark-Gluon Plasma - Relativistic HI - Beams Nuclear phase diagramCompressed nuclear/strange matterDeconfinement and chiral symmetry
Physics of Dense Plasmas and Bulk Matter - Bunch CompressionProperties of high density plasmasPhase transitions and equation of stateLaser - ion interaction with and in plasmas
Ultra High EM-Fields and Applications - Ions & Petawatt LaserQED and critical fieldsIon - laser interactionIon - matter interaction
SIS 18
Ion BeamHeating
Jupiter
Sun Surface
Magnetic Fusion
solid statedensity
Tem
pera
ture
[eV
]
Density [cm-3]
LaserHeating
PHELIX
Ideal plasmas
Strongly coupled
plasmas
Sun Core
InertialCofinement
Fusion
Primary Beams
•1.5-2 GeV/u; 238U28+, 1012/s;•35 GeV/u, 238U73+ 1010/s•30 GeV protons 4x1013/s
Secondary Beams
•radioactive beams, factor 104
intensity •Antiprotons 3 - 30 GeV
Storage and Cooler Rings
•Radioactive beams•e – A collider
•antiprotons 0.8 - 14.5 GeV 1011 stored and cooled
The New Facility and its Characteristics
• Rapidly cycling superconducting magnets• Cooled beams
Key Technical Features
Existing New
SIS 100/300
UNILAC
SIS 18
ESR
HESR
CR
NESR
Super FRS
STI-FAIRScientific + Technical Issues
Sidney Gales
AFI-FAIRAdministrative + Funding Issues
H.F.Wagner
ISC-FAIRInternat. Steering Committee
H.Schunck
PAC QCD
PAC NUSTAR
PAC APPA
TAC
Observer
FAIR Projekt
The Multi-National FAIR Project
J. Eschke 2004
Financing FAIR
Total cost: 675 M €, (TDR)recent update 1 Mrd € (increase of prices)
German govermnent: 65%State of Hesse: 10%
International Partners: 25%
Final decision on construction of FAIRafter commitment of partner statesto contribute 25% of construcgtion cost
2004 2005 2006
MoU
Contract Development
Contract Negotiations
Closing
LoI's
Proposals / TR's
PAC's Technical Committee
TDR's
Signing of MoU
Phase I – Governed by MoU
Phase IIGoverned
bycontracts
• Technical reports (accelerators and Super FRS) and design reports (Proposed experiments) have been submitted
• Evaluation mid March 2005
Signing of Memorandum of Understanding (MoU)September 23, 2004 in Berlin
FAIR member countries:Germany, Finland, France, Italy, Russia, Spain, Sweden, UK, Greece
Observers:Hungary, Poland, India, China, USA
Stage 1: 2007 - 2010Civil Construction• Ringtunnel for double ring
synchrotron incl. technical buildings
• Buildings housing the SFRS, 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 2: 2008 - 2013
HESR
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+ to 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 for fundamental symmetries and interactions
Stage 3: 2010 - 2014Accelerator • 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
Planning of Civil Construction /Layout of Buildings
SIS100/300 Underground Tunnel
5 m
-24 m
Tunnel in Open-Pit Construction
Superconducting Magnets for SIS 100
• Collaboration: JINR (Dubna)• Iron Dominated (window frame type) superferric design• Maximum magnetic field: 2 T• Ramp rate: 4 T/s• Hollow-tube superconducting cable, indirectly cooled• Two-phase helium cooling
• Collaboration: JINR (Dubna)• Iron Dominated (window frame type) superferric design• Maximum magnetic field: 2 T• Ramp rate: 4 T/s• Hollow-tube superconducting cable, indirectly cooled• Two-phase helium cooling
Nuclotron Dipole
•Improvement of DC-field quality• 2D / 3D calculations
•Guarantee of long term mechanical stability (≥ 2108 cycles )
•concern: coil restraint in the gap, fatigue of the conductor
•Reduction of eddy / persistent current effects (field, losses)
•Improvement of DC-field quality• 2D / 3D calculations
•Guarantee of long term mechanical stability (≥ 2108 cycles )
•concern: coil restraint in the gap, fatigue of the conductor
•Reduction of eddy / persistent current effects (field, losses)
PAC on QCD: ASSIA Study of Spin-dependent Interactions with Antiprotons R.Bertini TorinoCBM Compressed Baryonic Matter Experiment P.Senger GSIDIRAC Tests of Low Energy QCD L.Nemenov JINR DubnaPANDA Strong Interaction Studies with Antiprotons U.Wiedner TSL UppsalaPAX 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 LMUFLAIR - A Facility for Low-energy Antiproton and Ion Research E. Wiedman TokyoAnti-deuteron Breeding in a Double Ring Collider W. Oehlert FZ-JülichSPARC Stored Particles in Atomic physics Research R. Schuch StockholmHEDGEHOB: High Energy Density matter GEenerated by Heavy-iOn Beams D. Varentsov DarmstadtApplications of Relativistic Ions in Radiobiology and Space Research M. Durante NapoliMaterials Research with Relativistic Heavy Ion Beams S. Klaumünzer HMIRadiative Properties of Warm Dense Matter F. B. Rosmej Marseille
Letters of Intent (LoI)
834 users
505 users
Letters of Intent (LoI)
PAC on Nuclear Structure and Nuclear Astrophysics (NUSTAR-PAC):
1.) Low Energy Branch (LEB) .Scheidenberger GSIHigh-resolution In-Flight Spectroscopy (HISPEC) J. Gerl GSIDecay Spectroscopy with Implanted Ion Beams (DESPEC) J. Woods EdinburghPrecision Measurements of very short-lived Nuclei using an Advanced Trapping System for highly-charged Ions (MATS) K.Blaum MainzLASER Spectroscopy for the Study of Nuclear Properties (LASPEC) W.Nörtershäuser GSINeutron Capture Measurements (NCAP) M.Heil FZKAntiprotonic 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 SPNPIExotic Nuclei Studied in Light-Ion Induced Reactions at the NESR Storage Ring (EXL) H. Emling GSIElectron-Ion Scattering in a Storage Ring (e-A Collider) (ELISe) H. Simon GSIAntiproton-Ion Collider: A Tool for the Measurement of Neutron and Proton rms radii of Stable and Radioactive Nuclei (pbarA) P. Kienle TUMSpectroscopy of Pionic Atoms with Unstable Nuclei (PIONIC) K. Itahashi Riken
619 users
Collaborations at Large SetupsHadron Physics with Antiproton BeamsPhysics of Nuclear Matter
CBM Collaboration (W.Mueller) PANDA Collaboration (H. Orth)
Nuclear Structure, Astrophysics,ReactionsNUSTAR Collaboration
Super FRS
The NUSTAR-Facility
Phase 1The Concept has been developed within FINA
SHE – Status and Perspectives
GSI
JINR
Nextat GSI
RIKEN
RIKEN:Discovery of element 113Roentgenium (Rg)
has been acceptedfor Z = 111
0.68 0.70 0.72 0.74 0.76 0.78 0.80 0.82 0.84 0.86 0.88 0.90 0.9210-1
100
101
102
103
104
105
106
107
108
109
27Al+236U
26Mg+238U
26Mg+232Th
22Ne+236U
16O+242Pu
51V+208Pb
124Sn+90Zr (3n)
124Sn+92Zr (3n)
124Sn+94Zr (3n)
124Sn+96Zr (3n)
86Kr+121Sb (3n)
86Kr+123Sb (3n)
40Ar+176Hf
40Ar+178Hf
40Ar+180Hf
19F+248Cm
24Mg+232Th
25Mg+232Th
48Ca+184W (3n)
48Ca+197Au (3n)
48Ca+208Pb (3n)
48Ca+180Hf (3n)
48Ca+176Yb (4n)
48Ca+209Bi
50Ti+208Pb
50Ti+209Bi
54Cr+208Pb54Cr+209Bi
70Zn+208Pb
64Ni+209Bi
64Ni+208Pb58Fe+209Bi
58Fe+208Pb
48Ca+208Pb
40Ar+238U
37Cl+238U48Ca+238U
48Ca+208Pb (4n)
48Ca+226Ra
48Ca+186W (4n)
22Ne+238U
18O+249Cf
22Ne+244Pu
22Ne+244Pu
18O+249Bk18O+248Cm
22Ne+238U
22Ne+232Th
16O+238U
13C+248Cm
exp
eri
me
nta
l cro
ss
se
cti
on
(p
b)
effective fissility
cold fusion (1n) w/ 208Pb & 209Bi tgt.s shell stabilized hot fusion (3n) hot fusion (3n-5n) w/ actinide targets
hot fusion (3n-4n) w/ 48Ca beams
22Ne+243Am22Ne+248Cm
22Ne+249Bk
26Mg+248Cm34S+238U
48Ca+244Pu
48Ca+243Am48Ca+245Cm
48Ca+248Cm48Ca+249Cf
48Ca+173Yb (4n)48Ca+172Yb (4n)
SHE Production Cross-Sections
22Ne
34S
26Mg
30Si
31P
27Al
48Ca
DL claims: 0.2-5 pb
Courtesy V. Koch
FINUPHY Supported
The Future of Superheavy Element ResearchFebruary 17 - 18, 2004 GSI, Darmstadt, Germany
S. Hofmann, 60th birthday
3rd Workshop onRecoil Separator for Superheavy Element Chemistry
August 27, 2004, GSI, Darmstadt, Germany
Develop Strategies for GSI Research and Strengthen the InfrastructureResults: GSI projects Intensity upgrade TASCA
New RFQ-structure:• gain of the duty factor• higher injection energy• increased acceptance
Additional 28 GHz-ion-source:• intensity gain of factor two• higher charge states for increased duty factor
LEBT – Laminated magnets:• redundance for ion sources• preparation for future pulse to pulse operation with different ion-species
50% duty factor intensity-gain factor x2
New Front-end for the High Charge -State Injector
GSIDarmstadt@
RECSEP
SHECHEM
TASCA
Gas-filled recoil separator with maximized transmission (efficiency) for transactinides (SHE; Z ≥ 104) from hot-fusion reactions with actinide targets, in particular for:
Chemical investigations of elements 104 – 116(Towars picobarn chemistry)
Nuclear structure and nuclear reaction investigations of the most n-rich nuclides
Matthias Schädel, GSI, NUSTAR Annual Meeting 2005
TASCATASCA : : TTransAActinide SSeparator and CChemistry AApparatus
GSIDarmstadt@
RECSEP
SHECHEM
TASCA
Beam Line + TASCATASCA (DQQ)
Dipole, 310
Quadrupoleshoriz. vertic.
Detectorchambers
Target
Differential pumping and beam collimating
Beam diagnosis
Beam diagnosis
Beam wobbler
Valvesslow fast
UNILACBeam
European Consortium of Stable Beams (ECOS)High Intensity Stable Beams (HISB) Mandate
"Its task will be to go through the physics case presented by the French community, identify collaborations as well as the technical requirements and prepare a document for NuPECC.
" Minutes, NuPECC Meeting, Orsay, April 23-24, 2004
Members Faiçal Azaiez (Chair) Giacomo De Angelis Rolf-Dieter Herzberg Sigurd Hofmann Rauno Julin Marie-Hélène Moscatello Anna Maria Porcellato Uli Ratzinger Meetings continue
The low energy nuclear structure community has well defined and promising
research programs for the future. Many of them are based on measurements to be carried out using higher intensity stable beams.
The in-beam studies will benefit from the high segmentation of new detection
Systems and from digital electronics, in order to allow the increase of beam intensity by one order to two orders of magnitude ( up to few 100pnA).
Other approaches using detection systems after a separator (focal plane)require a stable beam facility with very high intensities ( up to 100pA)
In all the cases a dedicated detection system is needed to run experiments with longer beam time.
Existing European facilities Legnaro, JYFL, GSI (unilac), Ganil (CSS1)
Projects of very high intensity injectors for SPES and SPIRAL2
ECOS Strategy
• At the meetings in Orsay (April 2004) and Legnaro October 2004) reports were given by the members of ECOS on the present status and future plans of their home accelerator facilities or main experimental work with respect to production and use of intensive beams of stable isotopes.
• It is planned in a next step at the meeting in Jyvaskylae early 2005 to use this collection of information and data for preparation of a report on a most efficient and economic way to prepare high intensive stable beams for use in experiments. This report will be presented to NuPECC.
•