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Hadronic Matter at High Baryon Density Claudia Höhne, GSI Darmstadt

Hadronic Matter at High Baryon Density

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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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Page 1: Hadronic Matter at High Baryon Density

Hadronic Matter at High Baryon Density

Claudia Höhne, GSI Darmstadt

Page 2: Hadronic Matter at High Baryon Density

2 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010

At the end of this meeting ….

… let’s look into the future:

Page 3: Hadronic Matter at High Baryon Density

3 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010

… near future

Page 4: Hadronic Matter at High Baryon Density

4 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010

… more distant future

Page 5: Hadronic Matter at High Baryon Density

5 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010

… more distant future

Page 6: Hadronic Matter at High Baryon Density

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

Page 7: Hadronic Matter at High Baryon Density

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).

Page 8: Hadronic Matter at High Baryon Density

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!

Page 9: Hadronic Matter at High Baryon Density

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

)]

Page 10: Hadronic Matter at High Baryon Density

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

Page 11: Hadronic Matter at High Baryon Density

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]

Page 12: Hadronic Matter at High Baryon Density

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=,) ?

Page 13: Hadronic Matter at High Baryon Density

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)

Page 14: Hadronic Matter at High Baryon Density

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

]

Page 15: Hadronic Matter at High Baryon Density

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!

Page 16: Hadronic Matter at High Baryon Density

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

Page 17: Hadronic Matter at High Baryon Density

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

Page 18: Hadronic Matter at High Baryon Density

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!

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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

Page 20: Hadronic Matter at High Baryon Density

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

Page 21: Hadronic Matter at High Baryon Density

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

Page 22: Hadronic Matter at High Baryon Density

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!

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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

Page 24: Hadronic Matter at High Baryon Density

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

Page 25: Hadronic Matter at High Baryon Density

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!

Page 26: Hadronic Matter at High Baryon Density

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!

Page 27: Hadronic Matter at High Baryon Density

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

Page 28: Hadronic Matter at High Baryon Density

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

Page 29: Hadronic Matter at High Baryon Density

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/ → +-

Page 30: Hadronic Matter at High Baryon Density

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)

Page 31: Hadronic Matter at High Baryon Density

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

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32 Claudia Höhne Strongly Interacting Matter under Extreme Conditions, Hirschegg 2010

Beam spot in Q6

… further analysis ongoing

Page 33: Hadronic Matter at High Baryon Density

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.)

Page 34: Hadronic Matter at High Baryon Density

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

Page 35: Hadronic Matter at High Baryon Density

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

Page 36: Hadronic Matter at High Baryon Density

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)

Page 37: Hadronic Matter at High Baryon Density

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

Page 38: Hadronic Matter at High Baryon Density

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

Page 39: Hadronic Matter at High Baryon Density

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

Page 40: Hadronic Matter at High Baryon Density

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 ]

Page 41: Hadronic Matter at High Baryon Density

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