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Experimental study of dense matter at RHIC

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RUN1(2000) Au Au at 130GeV. RUN2(2001-2) Au Au/pp at 200GeV. RUN3(2003) d ... well reproduced by thermal distribution with radial expansion (blast wave model) ... – PowerPoint PPT presentation

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Title: Experimental study of dense matter at RHIC


1
Experimental study of dense matter at RHIC
  • Y. Akiba (RIKEN Nishina Center)
  • YITP Symposium
  • 2008.03.04

2
Outline
  • Introduction
  • Freezeout/final state
  • Hadronization
  • Scaling of v2/v4
  • Jet quenching at high pT
  • Constraining model parameter from RAA
  • Modification of jet-correlation shapes
  • Ridge?
  • J/y suppression
  • Heavy quark suppression and flow
  • di-leptons
  • Thermal(?) photons

3
Relativistic Heavy Ion Collider
  • Located at BNL
  • The first collider of heavy ion
  • Top Energy
  • sNN1/2 200 GeV for Au-Au
  • total s1/2 40 TeV for AuAu
  • RHIC Operations
  • RUN1(2000) AuAu at 130GeV
  • RUN2(2001-2) AuAu/pp at 200GeV
  • RUN3(2003) dAu/pp at 200GeV
  • RUN4(2004) AuAu/pp at 200 GeV
  • AuAu at 62 GeV
  • RUN5(2005) CuCu/pp at 200 GeV
  • CuCu at 62 and 22 GeV
  • RUN6(2006) pp at 200 GeV, 62 GeV
  • RUN7(2007) AuAu at 200 GeV
  • RUN8(2008) dAu at 200 GeV

4
The RHIC Experiments
RHIC
5
Formation of dense partonic matter at RHIC
  • In 2005, four RHIC experiments published white
    papers that summarized the experimental results
    of the first three years of RHIC operation
  • In the white papers, RHIC experiments concluded
    that state of dense partonic matter is formed in
    AA collisions at RHIC
  • The conclusion is primarily based on the
    following three pieces of evidence
  • Strong suppression of high pT hadrons in AuAu
    (jet quenching)
  • Absence of suppression in dAu
  • Strong elliptic flow in AuAu
  • The next step is to investigate the property of
    the dense matter
  • In the following I review the experimental data
    from RHIC.
  • Due to my background, most of the data is taken
    from PHENIX

6
Hadronic phase/Freeze out
7
Hadron spectra thermal freeze-out and radial
flow
PRL72,014903 (PHENIX)
  • Hadron spectra are well reproduced by thermal
    distribution with radial expansion (blast wave
    model)
  • p/K/p spectra can be simultaneously fit with two
    parameters
  • Tfo freezeout temp.
  • bT expansion velocity
  • Fit results
  • Tfo 110 MeV
  • bT 0.8 (ltbTgt 0.6)

8
Particle ratios Chemical equillibrium
NPA757,184 (PHENIX White Paper)
  • Thermal model reproduces hadron ratios.
  • Tch 160 MeV, mB 30 MeV
  • Evidence for Chemical equillibrium

9
3D source imaging
arXiv0712.4372
reverse engineer the correlation function by an
input source function. The analysis suggests that
there is a long tail of the source
distribution Solutoin of the long-standing HBD
puzzle?
3D source imaging reconstructs source parameters
10
Hadronization
11
Scaling of v2 of hadrons
PRL98_162301
  • More data on v2(pT) of hadrons are accumulated
  • When v2/nq vs KET/nq (KETtransverse kinetic
    enery), all data points are on a universal curve,
    suggesting that v2 developed in partonic stage

12
More on the scaling of v2 phi flow
PRL99_052301
Phi meson (small interaction cross section) also
follows the number of quark (nq) scaling.
13
v4 - scales with v2
V4
V4/(nq)2
V4
pT (GeV/c)
KET /nq (GeV/c2)
KET (GeV/c2)
v2 scales with nq, v4 with nq2 partonic
degree of freedom
14
High pT hadrons --- energy loss in QGP
High pT hadron Jet modificaiton J/psi Heavy
quarks Dileptons Thermal photon
15
p0 pT spectra at vsNN 200 GeV
RAA measurements now extends to 20 GeV/c
16
RAA of hadrons and direct photon (AuAu 200GeV)
  • Same suppression pattern for p0 and h
    Consistent with parton energy loss and
    fragmentation in the vacuum
  • RAA for fs larger than ?0 RAA for 2 lt pT lt 5
    GeV/c. Why?
  • Ncoll scaling for direct g (except for highest pT
    point? Isospin effect?)

17
Quantitative analysis (model dependent)
arXiv0801.1665
Quantitative comparison with PQM model
18
Quantitative analysis (more)
Comparison with GRV model dNg/dy1400
arXiv0801.1665
19
RAA beam energy dependence (CuCu)
?? CuCu 22,62,200 GeV (Run 5)
arXiv0801.4555
g
  • Model calculations indicate quenching expected at
    ?sNN 22 GeV, but Cronin effect dominates
  • Species dependence to probe space/time of
    suppression

20
High pT hadrons --- energy loss in QGP
High pT hadron Jet modificaiton J/psi Heavy
quarks Dileptons Thermal photon
21
Jet correlation
Recoil particles to central arm
PRD74,072002
pp collisions at 200 GeV
High pT trigger p0 to central arm EMCAL
22
Modification of jet correlation
  • This is another surprise two particle of two
    high pT track (jet correlation) is modified in
    central AuAu collisions.
  • Many theory attempts to explain this effect, but
    no consensus reached yet.

AuAu
PRL97,052301 (2006)
23
More detailed study of jet correlation
PRL98_232302
24
h-h correlations - jet functions
unchanged near-side peak in the final jet
functions when moving away from Reaction plane,
indication for away side modification.
25
The Ridge?
Ridge
Jet
STAR QM2006
Bulk Medium
In QM2006, STAR shows that there is
Ridge, Enhancement in small Df and large Dh of
leading particle This is the latest surprise in
jet correlation in AuAu This becomes a hot topic
in QM2008
26
Is there Ridge? Apparently
  • In QM2008, both PHENIX and PHOBOS shows that they
    also see Ridge
  • However, I myself is still skeptical about it.
  • The cause can be different from medium response.
  • It is difficult to imagine that information can
    propagate for a wide rapidity gap.
  • Speculation is it residual of v2 due to
    non-linear interaction between jets and v2?

27
J/psi --- probe of deconfinement(?)
High pT hadron Jet modificaiton J/psi Heavy
quarks Dileptons Thermal photon
28
J/y suppression
  • A quark gluon plasma has been predicted to
    suppress J/? production
  • Interesting suppression patterns have been
    observed at lower energies at the CERN SPS (NA50,
    NA60)
  • Rapidity and transverse momentum provide
    additional model constraints

29
J/y in pp
PRL98_232002
  • Order of magnitude higher statistics than the
    previous measurement by PHENIX
  • Pt and rapidity distribution are determined
  • Baseline for J/y suppression in AA

30
J/y suppression in AuAu
PRL98_172301
  • High statistics measurement of J/y in AuAu in
    wide rapidity range
  • Mid-rapidty J/y ? ee
  • Forward rapidty J/y?mm
  • Strong suppression of J/y is observed
  • Consistent with the prediction that J/ys are
    destroyed in de-confined matter
  • Surprisingly, the suppression is stronger at
    forward rapidity than in mid-rapidity
  • J/y formation by recombination of charm pairs in
    deconfined matter?

31
RAuAu (run 4) RAuAu (run 7)
NEW
  • Forward rapidity only (for now)
  • More bins at higher centrality
  • Confirm the trend
  • RAA(y1.7) lt RAA(y0)

32
J/? dAu Cold Nuclear Matter
PRC77_024912 (just publised)
J/? RdAu 200 GeV
  • Increased Run 5 pp statistics (x10 Run 3) as
    baseline
  • Improved consistent pp and dAu analysis
  • Improved alignment, resolution, yield
    extraction,
  • Cancellation of systematic errors in RdAu
  • Result CNM Shadowing(EKS) ?Breakup 2.8
    mb
  • Consistent within errors with previous results
  • and with ?Breakup4.2/-0.5mb (SPS result)

1.7 -1.4
33
J/? AuAu CNM Effects
J/? RAuAu 200 GeV (Run4)
PRC77_024912
1.2 lt y lt 2.2
  • Large errors still (need Run 8 dAu, Run 7 AuAu)
  • Comparison suggests more forward suppression
    beyond CNM than at mid-rapidity
  • BUT models shown dont describe RdAu impact
    parameter dependence

34
J/? RAA CuCu and AuAu
J/? RAA 200 GeV
  • Approx 2x more J/? in CuCu sample than AuAu
    sample
  • More precise Npartlt100 info
  • Curves show RAA prediction from ad hoc CNM fit to
    RdAu separately at y0 and y gt 1.2
  • CNM from RdAu fit describes suppression for Npart
    lt 100.

arXiv0801.0220
  • RdAu constraints are not sufficient to say if
    suppression beyond cold nuclear matter is
    stronger at forward rapidity

35
RHIC run 8 dAu 30 x run 3 !
  • Lets wait for this run analysis before to say
    more about cold matter (and derive decent
    survival probabilities)

36
Heavy quarks
High pT hadron Jet modificaiton J/psi Heavy
quarks Dileptons Thermal photon
37
Open Charm via Semi-Leptonic Decays
Due to its heavy mass, charm can only be produced
in early stage of collision. It can be used as
probe of hot dense matter. Open charm can be
measured through single leptons
e
p0
D0
For example
K
m-
nm
38
Heavy flavor production in pp
Phys. Rev. Lett 97,252002 (2006)
  • Single electrons from heavy flavor (charm/bottom)
    decay are measured and compared with pQCD theory
  • The new data extends the pT reach to 9 GeV/c
  • FONLL pQCD calculation agree with the data

39
Heavy Flavor in AuAu
PRL98_172301
No suppression at low pT Suppression observed
for pTgt3.0 GeV/c, smaller than for light quarks.
40
Comparison with models RAA v2
PRL98_172301
  • Two models describes strong
  • suppression and large v2
  • Rapp and Van Hee
  • Moore and Teaney
  • From model comparison,
  • viscosity to entropy ratio h/s
  • can be estimated
  • DHQ 2pT 4 - 6
  • DHQ 6 x h/(ep) 6 x h/Ts
  • ? h/s (4/3 2)/4p
  • The estimate of h/s is close
  • to the conjectured bound
  • 1/4p from AdS/CFT

41
Bottom Measurement
pp 200 GeV Charm and bottom extracted via e-h
mass analysis
  • Charm and bottom spectra both ?x? above FONLL
    calculations
  • But ratio is in good agreement with FONLL

42
Is bottom also suppressed? Does it flow?
  • pp data indicates that a large contribution of b
    for pTgt2 GeV/c
  • The suppression in high pT is strong and new v2
    data suggest significant flow of HF electron in
    high pT
  • Is bottom also suppressed?
  • Does bottom also flows?

43
Low mass dileptons
High pT hadron Jet modificaiton J/psi Heavy
quarks Dileptons Thermal photon
44
Measured pp Mee compared to Cocktail
  • Cocktail filtered in PHENIX acceptance
  • Charm, Bottom, DY contributions from PYTHIA
  • Excellent agreement!

arXiv0802.0050
45
Heavy Quarks in pp from ee-
After subtraction of Cocktail -
Fit to acharm bbottom (with PYTHIA shape)
  • Good agreement with single e results
  • Also new analyses via e-h coincidences, single
    muons, and direct charm measurement

arXiv0802.0050
46
total cross section of charm and bottom
vs dependence of cross section with NLO
pQCD agrees with data
47
AuAu Mee compared to Cocktail
  • Data and Cocktail absolutely normalized
  • Cocktail normalized to AuAu measurements
  • Except ccbar
  • Low mass excess
  • 150 lt Mee lt 750 MeV
  • X 3.40.2(stat.) 1.3(syst.)0.7(model)

arXiv0706.3034
48
PT Dependence of AuAu Mee
  • Low Mass excess is a low pT enhancement
  • Huge excess at lowest pT
  • Late Phase info

49
Thermal photons --- probe of initial T
High pT hadron Jet modificaiton J/psi Heavy
quarks Dileptons Thermal photon
50
Thermal Photons from the hot matter
If the dense matter formed at RHIC Thermailzed,
it should emit thermal radiation. This is
black body radition from the hot matter and the
direct evidence of thermalization in early
stage The temperature of the matter can directly
measured from the spectrum of thermal
photon. Measurement is difficut since the
expected signal is only 1/10 of photons from
hadron decays
51
Enhancement of almost real photon
  • QM2005
  • Results from AuAu
  • QM2008
  • long awaited result from pp
  • important confirmation of method
  • pp
  • Agreement of pp data and hadronic decay cocktail
  • Small excess in pp at large mee and high pT
  • AuAu
  • data agree for mee lt50MeV
  • Clear enhancement visible above for all pT

PHENIX Preliminary
1 lt pT lt 2 GeV 2 lt pT lt 3 GeV 3 lt pT lt 4 GeV 4 lt
pT lt 5 GeV
52
Direct ? Yield from ?
  • Virtual ??with pT gtgt mee should be produced
    directly with a rate and mass distrib. that
    follows a Dalitz form fdir with MHad-gtoo
  • Extract Direct ? excess as fraction r of fdir
    needed to describe low mass excess
  • That direct ? fraction of inclusive ? (mostly
    ???and ?) should be the same as the real ?
    fraction of inclusive ?? (mostly ???and ?)

53
Fraction of direct photons
  • Fraction of direct photons
  • Compared to direct photons from pQCD
  • pp
  • Consistent with NLO pQCD
  • favors small µ
  • AuAu
  • Clear excess above pQCD

pp
AuAu (MB)
µ 0.5pT µ 1.0pT µ 2.0pT
54
Direct ? via ? for pp, AuAu
  • New pp result with ? method agrees with NLO
    pQCD predictions, and with statistical method at
    high pT
  • Confirmation of the method
  • For AuAu (QM05 result) there is a significant
    low pT excess above pp expectations
  • If the direct photon in the AuAu is thermal
    origin, the initial temperature of the matter can
    be determined

arXiv0801.xxxx
55
Summary
Towards an unified description of the entire time
evolution
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