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Hadronic Matter at High Baryon Density. Claudia Höhne, GSI Darmstadt. At the end of this meeting …. … let’s look into the future:. … near future. … more distant future. … more distant future. Outline. Introduction & Motivation QCD phase diagram → high baryon densities! - PowerPoint PPT Presentation
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Hadronic Matter at High Baryon Density
Claudia Höhne, GSI Darmstadt
2 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
At the end of this meeting ….
… let’s look into the future:
3 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
… near future
4 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
… more distant future
5 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
… more distant future
6 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Outline
• Introduction & Motivation
• QCD phase diagram → high baryon densities!
→ phase transitions (quarkyonic phase?), CP?
• high baryon density – hadron gas – phase transition?
• multistrange hadrons, centrality dependence of K/ ratio, K/ fluctuations, dileptons, charm production
• CBM experiment at SIS100 and SIS300
• feasibility studies
• detector R&D
7 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
The QCD Phase Diagram
[A. Andronic et al., arXiv:0911.4806 ]
• crossover between hadronic and deconfined phase at low B and high T
• freeze-out curve (T,B)
• high precision data from RHIC (and soon LHC)
• equilibration!
• phase diagram at high B ?
• quarkyonic phase?
• phase transition(s)?
• equilibration?
• critical point/ triple point?
• need for high precision data including rare probes!
A. Andronic et al., Nucl. Phys. A 772, 167 (2006).
8 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Future explorations
complete scan of the QCD phase diagram with modern, 2nd generation experiments on the horizon!
30A GeV
• RHIC beam energy scan- evolution of medium properties- “turn-off” of established signatures- search for CP and PT
• NA61 at SPS (2007 acc. by SPSC)- search for CP and PT in energy-system size scan
• both essentially limited to high yield observables- RHIC: energy dependent
• FAIR and NICA- new accelerator projects- FAIR: high intensities! → rare probes!
Field driven by experimental data!
9 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Chemical freeze-out: a different view
• high (net-)baryon and energy densities created in central Au+Au collisions
beam energy
max. /0
max [GeV/fm3]
time span
~FWHM
5 AGeV 6 1.5 ~ 8 fm/c
40 AGeV 12 > 10 ~ 3.5 fm/c
[J.
Ra
ndru
p, J
. C
leym
ans
PR
C7
4, 0
4790
1 (2
006
)]
10 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Limiting temperature at √sNN ~ 10 GeV
• chemical freeze-out (fit T, B, V): temperature saturates for √sNN > 10 GeV although energy density (and initial T) still increases
→ deconfinement phase boundary reached, additional energy goes into heating the QGP
• occurs at the same energy at which mesons start to carry the larger part of the entropy
[A. Andronic et al., Phys. Lett. B 673 (2009) 142] [H.Oeschler et al., J.Phys.G 32, 223 (2006)]
s/T
3
SIS
100
SIS
300
SIS
100
SIS
300
11 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Multistrange Hadrons
SIS
100
SIS
300
• thermal equilibration also at low energies (high B) in particular concerning multistrange hadrons?
[A. Andronic et al., Phys. Lett. B 673 (2009) 142]
12 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
HADES: Sub-threshold - production
[HADES: PRL103, 132301, (2009)]
YK
[HADES: arXiv: 0911.0516]
Ar+KCl reactions at 1.76A GeV
• - yield by appr. 1 order of magnitude higher than thermal yield
• strangeness exchange reactions like
(Y=,) ?
13 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
K/ ratio – centrality dependence
• K/ ratio in central Pb+Pb (Au+Au) collisions well described by thermal model
• centrality dependence?[PHENIX, PRC 69 (2004) 034909][STAR, PRC79 (2009) 034909]• high energies: fast rise and
saturation behavior well understood in terms of percolation [1] or Core-Corona model [2]
[1] CH, F. Pühlhofer, R. Stock, Phys. Lett. B 640 (2006) 96[2] K.Werner, PRL 98, 152301 (2007)
14 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
K/ ratio – centrality dependence• lower energies?
→ same shape of centrality dependence for √sNN > 17 GeV→ changing dependence for lower energies?!→ relation to hadron rescattering/ freeze out at phase transition?
• other strangeness carriers – in particular , ?
[black & red lines: CH, F. Pühlhofer, R. Stock, PLB 640 (2006) 96]
[KA
OS
, JPG
31 (2005) S
693][E
802, PR
C 60 (199
9) 044904]
[NA
49 preliminary, Q
M09
]
15 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
• particle ratio fluctuations as sign for 1st order phase transition or CP?
• no data below 20 AGeV beam energy
• interpretation of measurements under discussion
• one suggestion:
K/ fluctuations
[NA49, Phys.Rev.C79:044910,2009]scaling with Volume (Nch) or number of K (NK) in acceptance?
→ test with centrality dependence!
16 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
K/ Fluctuations
• different scaling for energy and centrality dependences
• additional contributions from fluctuating cluster sizes/ core-corona contributions?!
• K/ fluctuations might be dominated by number of kaons
NN
NN
N
N
N
N
K
K
K
KKdyn
,cov2
varvar22
/
[D. Kresan, CPOD 2009, arXiv:0908.2875]
22mixeddatadyn
NA49 preliminary
17 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Dileptons[C
ER
ES
: E
ur.P
hys.
J.C
41,
47
5 (2
005)
]
• dileptons as direct probe of the high density phase
• CERES at 40 and 158 AGeV beam energy: excess higher at lower energy → importance of baryon density!
• HADES at SIS18: study coupling to baryons!
preliminary
explains C+C!
HADES, arXiv: 0907.3690 – QM09
18 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Charm propagation
[HSD: O. Linnyk et al., Int.J.Mod.Phys.E17, 1367 (2008)] [SHM: A. Andronic et al., Phys. Lett. B 659 (2008) 149]
Propagation of produced charm quarks in the dense phase –quark like or (pre-)hadron like?
• charmonium to open charm ratio as indicator – measure both!• indications of collectivity?
• first charm measurements in A+A below 158 AGeV!
• aim at detailed information including phase space distributions, flow!
19 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
CBM @ FAIR
+ HADES
CBM and HADES at SIS 100 and SIS 300
• systematic exploration of high baryon density matter in A+A collisions from 2 – 45 AGeV beam energy with 2nd generation experiments
• explore the QCD phase diagram, chiral symmetry restauration
20 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Module 0:SIS100
Module 1:CBM Cave,APPA hall
Module 2:SFRS + R3BModule 3:
Anti-proton facilityModule 4:Low-E NUSTAR, NESR, FLAIR, APPA-cave
Module 5:RESR
HADES and CBM startversion at SIS 100
21 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Nuclear equation-of-state: What are the properties and the degrees-of-freedom of nuclear matter at neutron star core densities? Hadrons in dense matter: What are the in-medium properties of hadrons? Is chiral symmetry restored at very high baryon densities? Strange matter: Does strange matter exist in the form of heavy multi-strange objects? Heavy flavor physics: How ist charm produced at low beam energies, and how does it propagate in cold nuclear matter?
s
s
s
uud? Λ
Λ
Nuclear matter physics at SIS 100
22 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
CBM: Physics topics and Observables
Onset of chiral symmetry restoration at high B
• in-medium modifications of hadrons (,, e+e-(μ+μ-), D)
Deconfinement phase transition at high B • excitation function and flow of strangeness (K, , , , )• excitation function and flow of charm (J/ψ, ψ', D0, D, c)• charmonium suppression, sequential for J/ψ and ψ' ?
The equation-of-state at high B
• collective flow of hadrons• particle production at threshold energies (open charm)
QCD critical endpoint• excitation function of event-by-event fluctuations (K/π,...)
Systematics & precision!!
→ characterization of the created medium!
CBM Physics B
ook
submitt
ed!
23 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Particle multiplicity ∙ branching ratio for min. bias Au+Au collisions at 25 GeV (from HSD and thermal model)
SPS Pb+Pb 30 A GeV
Particle multiplicities
24 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
The CBM experiment• tracking, momentum determination, vertex reconstruction: radiation hard silicon pixel/strip detectors (STS) in a magnetic dipole field
• hadron ID: TOF (& RICH)• photons, 0, : ECAL
• electron ID: RICH & TRD suppression 104
• PSD for event characterization• high speed DAQ and trigger → rare probes!
• muon ID: absorber + detector layer sandwich move out absorbers for hadron runs
RICHTRD
TOF ECAL
magnet
absorber +
detectorsSTS + MVD
25 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
STS tracking – heart of CBM
Challenge: high track density: 600 charged particles in 25o @ 10MHz
Task
• track reconstruction: 0.1 GeV/c < p 10-12 GeV/c p/p ~ 1% (p=1 GeV/c)
• primary and secondary vertex reconstruction (resolution 50 m)
• V0 track pattern recognition
c = 312 m
radiation hard and fast silicon pixel and strip detectors
self triggered FEE
high speed DAQ and trigger
online track reconstruction!
fast & rad. hard detectors!
26 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Parallelization in CBM Reconstruction !
Vector SIMD
MultiThreading
NVIDIA CUDA
OpenCL
STS + + + +
MuCh + +
RICH + +
TRD + +
Vertexing +
Open Charm Analysis
+
+ March 2009+ October 2009
DELL Server with: DELL Server with: • Core i7/NehalemCore i7/Nehalem 22x(Xeon X5550 44x2.66 GHz, 8 MB L3 cache)• DDR3-1333 36 GB36 GB main memory• NVIDIA NVIDIA GTX 295 2x240 FPUs2x240 FPUs, 1792 MB• optional LRBLRB
• fast event reconstruction is a must for CBM!
27 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
CBM feasibility studies
• feasibility studies performed for all major channels including event reconstruction and semirealistic detector setup
J/ J/
di-electrons di-muons
' '
c
1010 events
D0
28 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Di-electrons at SIS300
pt < 0.2 GeV/c
• CBM has acceptance for di-electron pairs down to lowest pt and Minv
• feasibility study for central Au+Au collisions, 25 AGeV, 200k events
detected pairs
29 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Feasibility studies for CBM at SIS 100• charm production in pC collisions with 30 GeV/c p-beam!
• open charm: STS + dipole magnet, TOFcharmonium: STS, dipole magnet, reduced muon detector
• study charm production at threshold, cold nuclear matter effects, reference data for later A+A collisions
4 cut
eff = 11.6 %
6 J/ψ recorded in 1010 events (b=0) (3·104 J/ψ per week)
J/ → +-
30 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Sensor development:double-sided micro-strips, stereo angle 15o, pitch 60 μm300 μm thick, bonded toultra-thin micro-cables,radiation hardness
STS in thermalenclosure
Detector planes: ultra-light weight ladder structure
Prototypes (sensors, electronics, cables for beam tests:
Development of the Silicon Tracking System (STS)
31 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
D1, D2
tracker boards Q2, Q4, Q6
beam
boards D1 + D2
rotation around vertical axis 20 deg
STS demonstrators in testbeam @ GSI (Sep ’09)
with 4 n-XYTER chips fully reading out one CBM baby detector
reference tracking telescope
with 3 or 4 stations
32 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Beam spot in Q6
… further analysis ongoing
33 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Monolithic Acitive Pixel Sensors in commercial CMOS process1010 m2 pixels fabricated, > 99%, x ~ 1.5 – 2.5 m
Micro Vertex Detecor (MVD) DevelopmentArtistic view of the MVD
• mechanical system integration • material for cooling!→ material budget!• vacuum compatibility
die thinned to 50 mglued to support.IPHC, Strasbourg (M. Winter et al.)
34 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Sensors for the MVD
Monolithic Active Pixel Sensors(MAPS, also CMOS-Sensors)
• Invented by industry (digital camera)
• Modified for charged particle detection since 1999 by IPHC Strasbourg
• Also foreseen for ILC, STAR…
~ 1 µm
MAPS(2009)
~ 0.05% X0
1.5µm
MAPS(2003)
~ 0.1% X0
Digital camera with 8.2 MPixel – CMOS MAPS
Topic
Single point resolution
Material budget
Rad. hard. non-io.
Rad. hard. io
CBMwish list
~ 5µm
few 0.1% X0
~1012 neq/cm² > 3x1013 neq/cm²
Time resolution
> 1 MRad 200 kRad
>1013 neq/cm²
> 3 Mrad
~ 50 µs ~ 1 ms< 30 µs
35 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
The MVD-demonstrator test @ CERN (Nov. 2009)
• First test of MVD demonstrator at CERN-SPS (Nov ’09)
• two single sided modules operated in coincidence “MVD telescope”, stations can be correlated by time stamps
• noise of the modules was 25-35 electrons (as expected from lab)
• data analysis ongoing
4 x MIMOSA-20 4 x 640 x 320 pixel 30 x 30 µm² pixel Serial analog readout Vacuum compatible cooling
36 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
RICH development
• develop robust but very efficient and high performant RICH detector based on industrial available components
• adopt self-triggered readout electronics
mirror + mount
MAPMT (H8500, Hamamatsu)
37 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
Hamamatsu H8500
MAPMT beamtest for RICH @ GSI (Sep ’09)
• plexiglass radiator for Cherenkov light generation by protons
• self-triggered readout electronics based on the n-XYTER adopted to the PMT readout (attenuation!): negligible noise level if requiring beam coincidence
3.5 hits/events
→ single photon counting with self triggered readout!
→ further analysis ongoing
38 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
STSSTSGEMGEMRICHRICH
DABC + Go4, Slow Control DABC + Go4, Slow Control
TriggerTrigger S3+S4S3+S4
CBM beamtest @ GSI (Sep 2009)
• combined beam time CBM & PANDA • 9 days of ~ 2 hours beam per day • protons, 2.0 GeV, ~ 104 p/s
39 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
DAQ in September 2009 Test Beam
FEB4nxBT
ROC EthA
BSYNC-S
AUX
FEB4nxBT
ROC EthA
BSYNC-S
AUX
ROC EthA
BSYNC-S
AUX
BEAM.
DABC
OnlineAnalysi
sGo4
discr
RICH/MAPMT ROC
EthA
BSYNC-M
AUX
FEB1nxGenFEB1nxGen
GEM2VECC
Beam Tag/Trigger
ROC EthA
BSYNC-S
AUX
ROC EthA
BSYNC-S
AUX
FEB1nxGenFEB1nxGen
FEB1nxGen
D1
D2
GEM1VECC
FEB1nxGen
6 ROC's8 FEB's12 n-XYTER
• system test!
• self-triggered FEE for all detectors, event building based on time stamps
40 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
CBM@FAIR – high B, moderate T:
• exploration of QCD phase diagram at high baryon densities at SIS 100 and SIS 300 (2-45 AGeV beam energy)
• together with HADES unique possibility of characterizing properties of baryon dense matter
• implementation of increasingly realistic detector response in simulations, parallelization of event reconstruction, first physics performance studies
• detector R&D ongoing
• several beamtests in 2009:RPCSTS, GEM, RICHMVD
Summary
[A. Andronic et al., arXiv:0911.4806 ]
41 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010
CBM collaboration
Russia:IHEP ProtvinoINR TroitzkITEP MoscowKRI, St. Petersburg
China:Tsinghua Univ., BeijingCCNU WuhanUSTC Hefei
Croatia:
University of SplitRBI, Zagreb
Portugal: LIP Coimbra
Romania: NIPNE BucharestBucharest University
Poland:Krakow Univ.Warsaw Univ.Silesia Univ. KatowiceNucl. Phys. Inst. Krakow
Ukraine: INR, KievShevchenko Univ. , Kiev
Univ. MannheimUniv. MünsterFZ RossendorfGSI DarmstadtUniv. WuppertalCzech Republic:
CAS, RezTechn. Univ. Prague
Germany: Univ. Heidelberg, Phys. Inst.Univ. HD, Kirchhoff Inst. Univ. Frankfurt
Hungaria:KFKI BudapestEötvös Univ. Budapest
India:Aligarh Muslim Univ., AligarhIOP BhubaneswarPanjab Univ., ChandigarhGauhati Univ., Guwahati Univ. Rajasthan, JaipurUniv. Jammu, JammuIIT KharagpurSAHA KolkataUniv Calcutta, KolkataVECC KolkataUniv. Kashmir, SrinagarBanaras Hindu Univ., Varanasi
Norway:Univ. Bergen
Kurchatov Inst. MoscowLHE, JINR DubnaLPP, JINR Dubna
Cyprus: Nikosia Univ.
56 institutions, > 400 members Split, Oct 2009
LIT, JINR DubnaMEPHI MoscowObninsk State Univ.PNPI GatchinaSINP, Moscow State Univ. St. Petersburg Polytec. U.
Korea:Korea Univ. SeoulPusan National Univ.
France: IPHC Strasbourg