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Partonic EoS in HighEnergy Nuclear Collisions

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Identify and study the properties of matter (EOS) with partonic degrees of freedom. ... New results, year-4. Larger data sample (year-4) allows analysis at higher pT: ... – PowerPoint PPT presentation

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Title: Partonic EoS in HighEnergy Nuclear Collisions


1
Partonic EoS inHigh-Energy Nuclear
Collisions
Nu XuLawrence Berkeley National
Laboratory Many thanks to the symposium
organizers
2
Outline
  • Numbers about Nu Xu
  • Date of birth 5 (Henning Index)
  • Ph.D 1985 - 1990 Stony Brook
  • Postdoc 1990 - 1994 Stony Brook
  • .
  • HI 5

work uncertain
work question
work doubt
3
Outline
  • Introduction
  • - equation of state
  • - collectivity, local thermalization
  • - chemical freeze-out QCD phase diagram
  • Jet-quenching at RHIC
  • Bulk properties
  • - partonic collectivity from multi-strange
    hadrons
  • - hint of charm collectivity
  • Summary

4
QCD Phase Diagram
5
LGT Predictions
  • 1) Large increase in ?
  • a fast cross cover !
  • 2) Does not reach ideal,
  • non-interaction S. Boltzmann
  • limit !
  • many body interactions
  • Collective modes
  • Quasi-particles are necessary
  • 3) TC 170 MeV robust!
  • Z. Fodor et al, JHEP 0203014(02)
  • Z. Fodor et al, hep-lat/0204001
  • C.R. Allton et al, hep-lat/0204010
  • F. Karsch, Nucl. Phys. A698, 199c(02).

Lattice calculations predict TC 170 MeV
Strongly interacting quark-gluon Plasma - sQGP
6
Physical Goals at RHIC
Identify and study the properties of matter
(EOS) with partonic degrees of freedom.
Penetrating probes Bulk probes -
direct photons, leptons - spectra, v1,
v2 - jets and heavy flavor
- partonic collectivity -
fluctuations jets - observed
high pT hadrons (at RHIC, pT(min) gt 3 GeV/c)
collectivity - collective motion of observed
hadrons, not necessarily reached
thermalization among them.
7
STAR
AuAu/CuCu/dAu 200 GeV QGP pp
(polarized) 200/500 GeV ?g
8
STAR TPC
9
Au Au Collisions at 130 GeV
Central Event
10
Collision Geometry, Flow
z
x
Non-central Collisions
Number of participants number of incoming
nucleons in the overlap region Number of binary
collisions number of inelastic nucleon-nucleon
collisions Charged particle multiplicity ?
collision centrality Reaction plane x-z plane
11
Hadron Spectra from RHICpp and AuAu collisions
at 200 GeV
0-5
more central collisions
Multi-strange hadron spectra are exponential in
their shapes.
STAR white papers - Nucl.
Phys. A757, 102(2005).
12
Yields Ratio Results
  • In central collisions, thermal model fit well
    with ?S 1. The system is thermalized at RHIC.
  • Short-lived resonances show deviations. There is
    life after chemical freeze-out. RHIC
    white papers - 2005, Nucl. Phys. A757, STAR
    p102 PHENIX p184.
  • First paper PBM et al, Phys. Lett. B344,
    43(95).

13
QCD Phase Diagram
First paper PBM et al, Phys. Lett. B344,
43(95).
14
EOS Study Step I
  • In Au Au collisions
  • Hadron yields in the state of equilibrium -
    chemical freeze-out near the phase transition
    temperature
  • Step I probing the medium with hard
    interactions

15
Energy Loss in AA Collisions
leading particle suppressed
back-to-back jets disappear
pp Au Au
Nuclear Modification Factor
16
Jet-Quenching at RHIC
In central AuAu collisions hadrons are
suppressed and back-to-back jets disappear.
Different from pp and dAu collisions. Energy
density at RHIC ? gt 5 GeV/fm3 30?0 Parton
energy loss Bjorken 1982 (Jet
quenching) Gyulassy Wang 1992
17
Jet-like di-hadron Correlations
New results, year-4
  • Larger data sample (year-4)
  • allows analysis at higher pT
  • Emergence of the away side peak
  • Background negligible at higher pT,assoc
  • - quantify the amount of suppression. Tests the
    medium property
  • STAR Preliminary, QM05

8 lt pT,trig lt 15 GeV
18
Heavy Flavor Hadron Energy Loss
1) Non-photonic electrons decayed from - charm
and beauty hadrons 2) At pT 6
GeV/c, RAA(n.e.) RAA(h) contradicts to naïve
pQCD predictions
Partonic energy loss - strongly interacting
matter produced at RHIC! Energy loss mechanism
under study M. Gyulassy et al. Problem
isolation of Charm hadron contributions from
Beauty-hadrons
19
Hard-soft Interactions - Thermalization
Two sources of particles - hard hard scattering
products. - soft bulk medium constituents. -
Very different as seen in peripheral. Become
similar in central.
STAR, nucl-ex/0501016 / PRL 95, 120301(05).
near
ltpTgt (GeV/c)
Leading hadrons
from away-jets
away
Medium
from medium
- PID correlation analysis - Search for signal of
shock-wave.
20
EOS Study Step II
  • In Au Au collisions
  • Hadron yields in the state of equilibrium -
    chemical freeze-out near the phase transition
    temperature
  • (2) Partonic energy loss - tense
    interactions amongst partons, strongly
    interacting matter
  • Step II study bulk properties with collective
    observations

21
Equation of State / Hydrodynamics
Energy density ? GeV/fm3
EOS - the system response to the changes of the
thermal conditions - is fixed by its p and T (?).
  • Equation of state
  • EOS I relativistic ideal gas p ?/3
  • EOS H resonance gas p ?/6
  • EOS Q Maxwell construction
  • Tcrit 165 MeV, B1/4 0.23 GeV
  • ?lat1.15 GeV/fm3
  • P. Kolb et al., Phys. Rev. C62,
    054909 (2000).

22
Anisotropy Parameter v2
coordinate-space-anisotropy ?
momentum-space-anisotropy
y
py
x
px
Initial/final conditions, EoS, degrees of freedom
23
High-Energy Nuclear Collisions
  • jets
  • J/y, D
  • W
  • f
  • X
  • L
  • p, K, K
  • D, p
  • d, HBT

partonic scatterings? early thermalization?
Initial Condition - initial scatterings -
baryon transfer - ET production - parton
dof System Evolves - parton interaction -
parton/hadron expansion Bulk Freeze-out -
hadron dof - interactions stop
Q2
TC Tch Tfo
elliptic flow v2

radial flow bT
time
24
v2 at Low pT Region
P. Huovinen, private communications, 2004
  • Minimum bias data! At low pT, model result
    fits mass hierarchy well!
  • - Details does not work, need more flow in the
    model!

25
? -mesons Flow Partonic Flow
  • ?-mesons are very special
  • they do not re-interact in hadronic environment
  • they are formed via coalescence with thermal
    s-quarks
  • they show strong collective flow

  • STAR
    Preliminary QM05, M. Lemont, S. Blyth talks

26
Collectivity, Deconfinement at RHIC
  • - v2 of light hadrons and
  • multi-strange hadrons
  • - scaling by the number of
  • quarks
  • At RHIC
  • ? mT - NQ scaling
  • ? Partonic Collectivity
  • ? Deconfinement
  • PHENIX PRL91, 182301(03)
  • STAR PRL92, 052302(04), 95, 122301(05)
  • nucl-ex/0405022, QM05
  • S. Voloshin, NPA715, 379(03)
  • Models Greco et al, PRC68, 034904(03)
  • Chen, Ko, nucl-th/0602025

i ii
27
Hadronic Transport Model Results
uRQMD results show the particle type dependence
although the absolute amplitudes of v2 are a
factor of 2 or so too small! 1) At low pT
region mass ordering - feature of hydrodynamic
motion 2) Hadron type dependence at the
intermediate pT region - vacuum hadronic cross
sections used in the model.
Y. Lu et al., nucl-th/0602009
The observation of the NQ-scaling is unique, but
the explanation may not be!
28
Multi-strange Hadron Ratios
In heavy ion collisions at RHIC, up to pT 4
GeV/c, (model predicts 8 GeV/c) the strangeness
production is dominated by the thermal like
processes. Hwa and
Yang, nucl-th/0602024 STAR data QM05, SQM06
29
Thermal Model Fits
  • Source is assumed to be
  • Locally thermal equilibrated
  • Boosted radially

boosted
E.Schnedermann, J.Sollfrank, and U.Heinz, Phys.
Rev. C48, 2462(1993)
random
30
Blast Wave Fits Tfo vs. lt bT gt
  • 1) p, K, and p change
  • smoothly from peripheral
  • to central collisions.
  • 2) At the most central
  • collisions, ??T? reaches
  • 0.6c.
  • 3) Multi-strange particles ?,
  • ? are found at higher T
  • and lower ??T?
  • ? Sensitive to early partonic stage!
  • STAR NPA715, 458c(03) PRL 92, 112301(04) 92,
    182301(04).

200GeV Au Au collisions
Multi-strange hadrons freeze-out with higher Tfo
(Tch) and smaller ??T?
31
T vs. Mass Plot (SPS)
  • Interaction with hadronic gas
  • Large X-section limit
  • pions, kaons, protons
  • Small X-section limit
  • ?, ?, J/ ?

32
Slope Parameter Systematics
At RHIC, ?, ?, ?, and J/? show collective motion
in 200 GeV Au Au central collisions!

PHENIX (?, K, p, J/?) PRC69, 034909(04), QM05
STAR (?, ?, ?) QM05.
33
EOS Parameters at RHIC
In central AuAu collisions at RHIC -
partonic freeze-out Tpfo 165 10 MeV
weak centrality dependence vpfo 0.2 (c) -
hadronic freeze-out Tfo 100 5 (MeV)
strong centrality dependence vfo 0.6 0.05
(c) Systematic study are needed to understand
the centrality dependence of the EOS
parameters Thermalization assumed
34
EOS Study Step III
  • In Au Au collisions
  • Hadron yields in the state of equilibrium -
    chemical freeze-out near the phase transition
    temperature
  • (2) Partonic energy loss - tense
    interactions amongst partons, strongly
    interacting matter
  • (3) Partonic collectivity and
    de-confinement
  • Step III test thermalization with heavy flavor
    hadrons

35
Open-/Closed-charm Hadron Yields
A. Andronic, P. Braun-Munzinger, K. Redlich, J.
Stachel, Phys.Lett. B571 , 36(03).
T. Matsui and H. Satz, Phys. Lett. B178,
416(1996). L. Grandchamp and R. Rapp, Phys. Lett.
B523 , 60(01).
RHIC
RHIC
(1) open charm cross sections (3) medium
effects (? properties) (2) direct pQCD
production (4) absorption (color
screening) Model results are different,
centrality dependence measurements are important!
36
Charm Cross Section Results
First set of measurements, systematic errors are
large. Precision data are needed - energy loss
analysis ? test pQCD in hot and dense medium -
J/? analysis ? test Charm thermalization and
de-confinement
37
QCD Phase Diagram
phase boundary? (hadronic shore)
deep partonic ocean
LHC RHIC-II
RHIC energy scan CBM at GSI
Tpfo 16510 MeV vpfo 0.2 (c)
Tfo 1005 MeV vfo 0.60.05 (c)
38
WORK
  • Each soul is potentially divine. The goal is
    to manifest this divinity within by controlling
    nature external and internal. Do this either by
    work, or worship, or psychic control, or
    philosophy - by one, or more, or all of these -
    and be free.''
  • -- Swami Vivekananda

39
Happy Birthday! ??????,??!
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