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Heavy ion collisions and AdS/CFT
Amos Yarom
With S. Gubser and S. Pufu.
Part 1:
Shock waves and wakes.
RHIC
Au
79 protons
118 neutrons
197 nucleons
En = 100 GeV
~ En/Mn ~ 100
RHIC
Au
79 protons
118 neutrons
197 nucleons
En = 100 GeV
~ En/Mn ~ 100
RHIC
t < 0
RHIC
t > 0
~ 5000
RHIC
ddN
RHIC
ddN
0
STAR, nucl-ex 0701069
RHIC
ddN
0
RHIC
ddN
0
RHIC
RHIC
cs/v=cos
ddN
0
RHIC
ddN
0
Casalderrey-Solana et. al. hep-ph/0411315
ddN
0
I
I
II
II
Casalderrey-Solana et. al. hep-ph/0411315
I II
AdS space
z
0
AdS-Schwarzschild
z
0
z0
AdS-Schwarzschild
What we expect for the stress tensor:
Conformal invariance:
Large N:
So:
AdS-Schwarzschild
Computing the stress tensor:
Rewrite the metric in the form:
The boundary theory stress tensor is given by:
AdS-SchwarzschildTo convert from the z to the y coordinate system:
Recall that we need: So we can compute:
AdS-SchwarzschildFrom: and
We find:
Using the AdS/CFT dictionary:
We obtain:
AdS-Schwarzschild
z
0
z0
A moving quark
z
0
z0
?
Consider a `probe quark’. It’s profile will be given by the solution to the equations of motion which follow from:
A quark is dual to a string whose endpoint lies on the boundary
A moving quark
Consider the ansatz:
We can easily evaluate:
The string metric is:
A moving quark
A moving quark
Notice that since the Lagrangian is independent of , then
is conserved. Inverting this relation we find:
A moving quark
Requiring that implies that the numerator and
denominator change sign simultaneously.
Defining:
Then:
A moving quark
z
0
z0
? v
The metric backreactionThe total action is
The equations of motion are:
where:
+ equations of motion for the string.
The metric backreaction
where:
The AdS/CFT dictionary gives us:
So
We work in the limit where:
The metric backreaction
where:
We work in the limit where:
The metric backreaction
We work in the limit where:
To leading order:
Whose solution is
The metric backreaction
We work in the limit where:
Whose solution is
The metric backreaction
We make a few simplifications:•Work in Fourier space:
•Fix a gauge:
At the next order:
•Use the symmetries:
The metric backreaction
We eventually must resort to Numerics. Using:
we can obtain:
At the next order:
Energy density
Energy density
Energy density
Near field energy density
The Poynting vector
I II
Some universal properties
They also remain unchanged if the string is replaced by another object that goes all the way to the horizon.
These results remain unchanged even if we add scalar matter,
I II
Noronha et. al. Used a hadronization algorithm to obtain an azimuthal distribution of a “hadronized” N=4 SYM plasma.
References• STAR collaboration nucl-ex/0510055, PHENIX collaboration 0801.4545. Angular correlations.
• Casalderrey-Solana et. al. hep-ph/0411315. Shock waves in the QGP.
• Gubser hep-th/0605182, Herzog et. al. hep-th/0605158. Trailing strings.
• Friess et. al. hep-th/0607022, Yarom. hep-th/0703095, Gubser et. al. 0706.0213, Chesler et. al. 0706.0368, Gubser et. al. 0706.4307, Chesler et. al. 0712.0050. Computing the boundary theory stress tensor.
• Gubser and Yarom 0709.1089, 0803.0081. Universal properties.
• Noronha et. al. 0712.1053, 0807.1038, Betz et. al. 0807.4526. Hadronization of AdS/CFT result.
• Gubser et. al. 0902.4041, Torrieri et. al. 0901.0230 Reviews.