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What do we learn from

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Roy A. Lacey. What do we learn from. Correlation ... Roy A. Lacey, Stony Brook, ... Roy A. Lacey, Stony Brook, ISMD, Kromer , 2005. 16. Does the Flow follow ... – PowerPoint PPT presentation

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Title: What do we learn from


1
What do we learn from Correlation measurements at
RHIC
2
Motivation
Which observables phenomena connect to the
de-confined stage?
3
Flow correlations provide an important probe
4
Prologue
Low Energy Squeeze-out
High Energy In-plane
Do we understand Flow correlations ?
Pressure Gradients Drive Transverse and Elliptic
flow
The expected transition Is observed
Phys.Rev.Lett.831295,1999
5
What information do Flow correlations provide?
  • Provides reliable estimates of pressure
    pressure gradients
  • Can address questions related to thermalization
  • Gives insights on the transverse dynamics of the
  • medium
  • Provides access to the properties of the medium
  • - EOS, sound speed (cs ), viscosity, etc

6
There are two sources of azimuthal correlations
at RHIC !
Azimuthal Correlations Provide Two Direct routes
to the Properties of the High Energy Density
Matter Created at RHIC
7
Reminder High Energy density matter is created at
RHIC!
The Energy Density is Well Above the Predicted
Value for the Phase Transition /crossover !
8
Reminder Particle production system size
Un-scaled dN/d?
PHOBOS Data
Particle production is essentially geometry
dominated
9
Reminder Statistical Model Comparisons of
Particle Ratios
Hadro-chemistry indicates a single Hadronization
Temperature 175 MeV
10
Is Thermalization Rapid ?
Self quenching
Substantial elliptic flow signals should be
present for a variety of particle species
11
Is Thermalization Rapid ?
Large Pressure Gradients are Generated Very Early
!
12
v2 sheet for mesons Baryons
Exquisite Features Due to Radial flow ?
13
Is Thermalization Rapid ?
Heavy quark Thermalization ?
14
Is the matter unique ?
CERES
Results are strikingly similar for
V2 decreases by 50 from RHIC to SPS
Significantly larger pressure (gradients) at RHIC
than at SPS
15
Excitation function for differential v2
Apparent saturation of v2 for
Possible indication for a soft EOS !
16
Does the Flow follow ideal hydrodynamics ?
Non-trivial issue for EOS, viscosity, etc
Investigate Hydrodynamic Scaling Relations for
the fine structure of v2
Fit Data
17
Fine Structure Scaling
Note Universal Scaling prediction
M. Csanad C. Csörgo et al.
18
Scaling Tests
Eccentricity scaling
19
Scaling of azimuthal anisotropy - Mesons
PHENIX Preliminary
PHENIX Preliminary
  • Scaling works over a broad range for charged
    hadrons
  • and identified particles

20
Scaling of azimuthal anisotropy - Hydro
Hydro eccentricity scaling
21
Scaling of azimuthal anisotropy - system size
PHENIX Preliminary
Scaling of CuCu and AuAu collisions indicate
system size indipendece
22
Scaling PHENIX Data
PHENIX Preliminary
5ltCentralitylt30
  • Unequivocal scaling at low values
  • scaling breaks 1.8

23
Scaling of azimuthal anisotropy - hadrons
Integral flow scaling observed across
24
Scaling of RHIC data
  • Demonstration of higher harmonic scaling

25
Scaling of RHIC data
  • Demonstration of Comprehensive scaling at RHIC

26
Quark number scaling -- Partonic Flow ?
baryons
?? OO ?
mesons
200 GeV AuAu
Hadronic re-scattering does not support observed
Phi flow !
27
Extended Fine Structure scaling
PHENIX Preliminary
5ltCentralitylt30
All Flow Data Now Understood
Universal scaling prediction!
28
Scaling of azimuthal anisotropy - Hydro
Estimate cs !
29
Initial Foray
  • Fits to the data can provide estimates of the
    properties of the produced matter

30
Epilogue
Correlation measurements give compelling
evidence for the production of strongly
interacting high energy density partonic matter
in RHIC collisions.
sQGP
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