Collective Flow Art Poskanzer Exploring the secrets of the universe
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Transcript Collective Flow Art Poskanzer Exploring the secrets of the universe
Collective Flow
Art Poskanzer
Exploring the secrets
of the universe
1
Color by Roberta Weir
Photos
macroscopic nuclear physics
Poskanzer, Swiatecki, 1982
and Seaborg
(1986)
1998
2
Spectator-Participant Picture
1973
Abrasion and Ablation of Heavy Ions,
3 J.D. Bowman, W.J. Swiatecki, and C.F. Tsang, LBL-2908 (1973)
Fireball
4
G.D. Westfall et al., Phys. Rev. Letters 37, 1202 (1976)
Centrality Dependence
Peripheral Collision
z
y
Y
(near) Central Collision
x
Y
X
5
z
y
x
X
Transverse Plane
Transverse Plane
y
x
H. Wieman (2005)
around the beam axis
<y2> - <x2>
ε=
<y2> + <x2>
6
Danielewicz
S=πxy
Elliptic Flow
QuickTime™ and a
YUV420 codec decompressor
are needed to see this picture.
7
Animation by Jeffery Mitchell (Brookhaven National Laboratory)
Nuclear Collisions
1975
Mass
Bevalac
Energy in cm
Explored to date only on the axes.
8
W.J. Swiatecki, Bevalac Upgrade Proposal, 1975.
SPS
RHIC
Kinds of Flow
mainly spectator matter
self quenching
early time
temperature
9
Plateau
1984
Temperature
or Pressure
direct photons
elliptic flow
Beam Energy
10
W. Swiatecki (1984)
v2 /
11
NA49,
C. Alt etand
al.,A.M.
Phys.Poskanzer,
Rev. C 68 Phys.
034903
(2003)
S.A. Voloshin
Letters
B 474, 27 (2000)
Azimuthal Flow Angle
py
px
12
S. Voloshin and Y. Zhang, Z. Phys. C 70, 665 (1996)
Fourier Harmonics
Event plane resolution correction made for each harmonic
Unfiltered theory can be compared to experiment!
Voloshin
S. Voloshin and Y. Zhang, hep-ph/940782; Z. Phys. C 70, 665 (1996)
See also, J.-Y. Ollitrault, arXiv nucl-ex/9711003 (1997)
13 and J.-Y. Ollitrault, Nucl. Phys. A590, 561c (1995)
Methods of Analysis
14
Pair-wise
Standard
Scalar Product
q-dist
Cumulant
Lee-Yang Zeros
Directed and Elliptic Flow at the SPS
pions
y
pt
15 NA49, C. Alt et al., PRC 68, 034903 (2003)
protons
STAR
QuickTime™ and a
YUV420 codec decompressor
are needed to see this picture.
16
First RHIC Elliptic Flow
First paper from STAR
130 GeV/A Au+Au
22 k events
hydro
Data approach hydro
for central collisions
Snellings
17
Voloshin
Poskanzer
STAR, K.H. Ackermann et al., PRL 86, 402 (2001)
Elliptic Flow vs. Beam Energy
25% most central
mid-rapidity
all v2
bounce-off
In-plane
elliptic flow
squeeze-out
six decades
18 A. Wetzler (2005)
Directed Flow from Mixed Harmonics
2nd har. event plane
N-particle cumulants
v1{EP1,EP2}
v1{3}
Removes nonflow
Uses best determined event plane
19
STAR, J. Adams et al., PRC submitted (2005)
v1 from Spectator Neutrons
Zero-Degree Calorimeter Shower Max Detector
for transverse deflection of spectator neutrons
20
A. Tang, STAR
Quark Coalescence
n = number of
constituent quarks
D. Molnar and S.A. Voloshin, Phys. Rev. Letters 91, 092301 (2003)
21 STAR, Phys. Rev. C 72, 014904 (2005)
Higher Harmonics
vn = 1.2 v2n/2
more details of the event shape in p space
quarks have v4
22 J. Adams et al., PRL 92, 062301 (2004)
Conclusions from Flow
Hydrodynamics at top RHIC Energy
Parton Coalescence
Partonic Phase
Thermalized Partonic Phase
23
Thermalization
Quark-Gluon Plasma