early time evolution of high energy nuclear collisions
DESCRIPTION
Early Time Evolution of High Energy Nuclear Collisions. Rainer Fries Texas A&M University & RIKEN BNL. With J. Kapusta and Y. Li. Early Time Dynamics in Heavy Ion Collisions McGill University, Montreal, July 18, 2007. Motivation. How much kinetic energy is lost in the collision of - PowerPoint PPT PresentationTRANSCRIPT
Early Time Evolution of High Energy Nuclear
Collisions
Rainer FriesTexas A&M University & RIKEN BNL
Early Time Dynamics in Heavy Ion CollisionsMcGill University, Montreal, July 18, 2007
With J. Kapusta and Y. Li
ETD-HIC 2 Rainer Fries
Motivation
ETD Questions
ETD IdeasQGP
HydroclQCDCGC
pQCD
How much kinetic energy is lost in the collision of two nuclei with a total kinetic energy of 40 TeV? How long does it take to decelerate them?
How is this energy stored initially?Does it turn into a thermalized plasma?How and when would that happen?
Pheno.Models
ETD-HIC 3 Rainer Fries
PCM & clust. hadronization
NFD
NFD & hadronic TM
PCM & hadronic TM
CYM & LGT
string & hadronic TM
Motivation
Assume 3 overlapping phases:1. Initial interaction: energy deposited between the nuclei;
gluon saturation, classical fields (clQCD), color glass2. Pre-equilibrium / Glasma: decoherence? thermalization?
particle production? instabilities?3. Equilibrium (?): (ideal ?) hydrodynamics
What can we say about the global evolution of the system up to the point of equilibrium?
HydroNon-abeliandynamicsclQCD
ETD-HIC 4 Rainer Fries
Outline
Goal: space-time map of a high energy nucleus-nucleus collision.
Small time expansion of YM; McLerran-Venugopalan model
Energy density, momentum, flow
Matching to Hydrodynamics
Baryon Stopping
ETD-HIC 5 Rainer Fries
Hydro + Initial Conditions
Hydro evolution of the plasma from initial conditions Energy momentum tensor for ideal hydro
+ viscous corrections ? e, p, v, (nB, …) have initial values at = 0
Goal: measure EoS, viscosities, … Initial conditions = additional parameters
Constrain initial conditions: Hard scatterings, minijets (parton cascades) String or Regge based models; e.g. NeXus [Kodama et al.]
Color glass condensate [Hirano, Nara]
v,1 u pguupexT ,,pl
ETD-HIC 6 Rainer Fries
Hydro + Initial Conditions
Hydro evolution of the plasma from initial conditions Energy momentum tensor for ideal hydro
+ viscous corrections ? e, p, v, (nB, …) have initial values at = 0
Assume plasma at 0 created through decay of gluon field F with energy momentum tensor Tf
. Even w/o detailed knowledge of non-abelian dynamics:
constraints from energy & momentum conservation for Tpl
Tf !
Need gluon field F and Tf at small times.
Estimate using classical Yang-Mills theory
v,1 u pguupexT ,,pl
ETD-HIC 7 Rainer Fries
Classical Color Capacitor
Assume a large nucleus at very high energy: Lorentz contraction L ~ R/ 0 Boost invariance
Replace high energy nucleus by infinitely thin sheet of color charge Current on the light cone Solve classical Yang Mills equation
McLerran-Venugopalan model: For an observable O: average over charge distributions Gaussian weight
JFD ,
x11 xJ
2
22
2exp
xxdOdO
[McLerran, Venugopalan]
ETD-HIC 8 Rainer Fries
Color Glass: Two Nuclei
Gauge potential (light cone gauge): In sectors 1 and 2 single nucleus solutions Ai
1, Ai2.
In sector 3 (forward light cone):
YM in forward direction: Set of non-linear differential
equations Boundary conditions at = 0
given by the fields of the single nuclei
xAA
xAxAii ,
,
0,,,1
0,,1
0,,1
2
33
jijii
ii
ii
FDADAigA
AAigAD
ADDA
xAxAig
xA
xAxAxA
ii
iii
21
21
,2
,0
,0
22 zt
iA1iA2
[McLerran, Venugopalan][Kovner, McLerran, Weigert][Jalilian-Marian, Kovner, McLerran, Weigert]
ETD-HIC 9 Rainer Fries
Small Expansion
In the forward light cone: Perturbative solutions [Kovner, McLerran, Weigert]
Numerical solutions [Venugopalan et al; Lappi]
Analytic solution for small times? Solve equations in the forward light cone using
expansion in time : Get all orders in coupling g and sources !
xAxA
xAxA
in
n
ni
nn
n
0
0
,
,
YM equations
In the forward light cone
Infinite set of transverse differential equations
ETD-HIC 10 Rainer Fries
Solution can be found recursively to any order in !
0th order = boundary condititions:
All odd orders vanish
Even orders:
Small Expansion
422
2
,,,1
,,2
1
nmlkm
ilk
nlk
jil
jk
in
nmlkm
il
ikn
ADAigFDn
A
ADDnn
A
xAxAig
xA
xAxAxA
ii
iii
210
210
,2
ETD-HIC 11 Rainer Fries
Note: order in coupled to order in the fields.
Expanding in powers of the boundary fields : Leading order terms can be resummed in
This reproduces the perturbative KMW result.
Perturbative Result
kJAA
kJk
AA
ii00
LO
10LO
,
2,
kk
kk
ii AA 21 ,
In transverse Fourier space
ETD-HIC 12 Rainer Fries
Field strength order by order: Longitudinal electric,
magnetic fields start with finite values.
Transverse E, B field start at order :
Corrections to longitudinal fields at order 2.
Corrections to transverse fields at order 3.
Gluon Near Field
jiij
ii
AAigF
AAigF
21210
210
,
,
E0
B0
0000)1( ,,22
FDFDe
F ijiji
☺
☺
ETD-HIC 13 Rainer Fries
Gluon Near Field
Before the collision: transverse fields in the nuclei E and B orthogonal
ii AxF 11
ii AxF 22
ETD-HIC 14 Rainer Fries
Gluon Near Field
Before the collision: transverse fields in the nuclei E and B orthogonal
Immediately after overlap: Strong longitudinal electric,
magnetic fields at early times0E
0B
ETD-HIC 15 Rainer Fries
Gluon Near Field
Before the collision: transverse fields in the nuclei E and B orthogonal
Immediately after overlap: Strong longitudinal electric,
magnetic fields at early times
Transverse E, B fields start to build up linearly
iE
iB
ETD-HIC 16 Rainer Fries
Gluon Near Field
Reminiscent of color capacitor Longitudinal magnetic field of ~ equal strength
Strong initial longitudinal ‘pulse’: Main contribution to the energy momentum tensor
[RJF, Kapusta, Li]; [Lappi]; …
Particle production (Schwinger mechanism) [Kharzeev, Tuchin]; ...
Caveats: Instability from quantum fluctuations? [Fukushima, Gelis,
McLerran]
Corrections from violations of boost invariance?
ETD-HIC 17 Rainer Fries
Energy Momentum Tensor
Compute energy momentum tensor Tf.
Initial value of the energy density:
Only diagonal contributions at order 0:
Longitudinal vacuum field
Negative longitudinal pressure maximal anisotropy transv. long. Leads to the deceleration of the nuclei
Positive transverse pressure transverse expansion
20
20
000f0 2
1BET
0
0
0
0
)0(f
T
ETD-HIC 18 Rainer Fries
Energy Momentum Tensor
Energy and longitudinal momentum flow at order 1:
Distinguish hydro-like contributions and non-trivial dynamic contributions
Free streaming: flow = –gradient of transverse pressure
Dynamic contribution: additional stress
coshsinh2
1
sinhcosh2
1
31
01
iii
iii
T
T
0 ii
0000 ,, BEDEBD jjiji
ETD-HIC 19 Rainer Fries
Energy Momentum Tensor
Order O( 2): first correction to energy density etc.
General structure up to order 3 (rows 1 & 2 shown only)
Energy and momentum conservation:
..coshsinh16
coshsinh2
2cosh2sinh8
..4
sinhcosh16
sinhcosh2
..4
sinhcosh16
sinhcosh2
..sinhcosh16
sinhcosh2
2sinh2cosh84
113
10
12
222
32
02
10
2
011
31
01
113
10
12
0
2
0
f
ii
ii
T
0,3)( 0
1,2)( 03
f
4f
iOT
iOT
ETD-HIC 20 Rainer Fries
McLerran Venugopalan Model
So far just classical YM; add color random walk.
E.g. consider initial energy density 0.
Correlator of 4 fields, factorizes into two 2-point correlators:
2-point function Gk for nucleus k:
Analytic expression for Gk in the MV model is known. Caveat: logarithmically UV divergent for x 0! Not seen in previous numerical simulations on a lattice. McLerran-Venugopalan does not describe UV limit correctly;
use pQCD
00~~ 2121210 GGAAAA lkjiklijklij
xAAxG ik
ikk 0
[T. Lappi]
ETD-HIC 21 Rainer Fries
Estimating Energy Density
Initial energy density in the MV model
Q0: UV cutoff
k2: charge density in nucleus k from
Compatible with estimate using screened abelian boundary fields modulo exact form of logarithmic term. [RJF, Kapusta, Li (2006)]
2
2022
221
26
0 ln8
1
QNNg cc
yxgyx kak
ak
222
ETD-HIC 22 Rainer Fries
Compare Full Time Evolution
Compare with the time evolution in numerical solutions [T. Lappi]
The analytic solution discussed so far gives:Normalization Curvature
Curvature
Asymptotic behavior is known (Kovner, McLerran, Weigert)
T. Lappi
Bending around
ETD-HIC 23 Rainer Fries
Transverse Flow @ O(1)
Free-streaming part in the MV model.
Dynamic contribution vanishes!
2
2022
221
26
ln8
1
QNNg icci
0i
ETD-HIC 24 Rainer Fries
Anisotropic Flow
Sketch of initial flow in the transverse plane:
Clear flow anisotropies for non-central collisions! Caveat: this is flow of energy.
b = 8 fm
iT 0free
b = 0 fm
iT 0free
ETD-HIC 25 Rainer Fries
Coupling to the Plasma Phase
How to get an equilibrated plasma?
Use energy-momentum conservation to constrain the plasma phase Total energy momentum tensor of the system:
r(): interpolating function
Enforce
rTrTT 1plf
fT
plT
0 T
ETD-HIC 26 Rainer Fries
Coupling to the Plasma Phase
Here: instantaneous matching I.e. Leads to 4 equations to constrain Tpl. Ideal hydro has 5 unknowns: e, p, v
Analytic structure of Tf as function of
With etc…
Matching to ideal hydro only possible w/o ‘stress’ terms
0r
53
162
OV iii
2sinh2coshcoshsinh2sinh2cosh
coshsinhsinhcosh
2sinh2coshsinhcosh2sinh2cosh
f
CBBAWVCB
WVWV
CBWVCBBA
Tii
iiii
ii
ETD-HIC 27 Rainer Fries
The Plasma Phase
In general: need shear tensor for the plasma to match.
For central collisions (use radial symmetry):
Non-vanishing stress tensor: Stress indeed related to pr = radial pressure
Need more information to close equations, e.g. equation of state
Recover boost invariance y = (but cut off at *)
tanhv
v
22
z
rr
r
rr
pA
V
pA
VpApe
162
8
24
3
0
2
0
2
0
rV
C
A
ii
22 VpAV
Cr
rz
Small times:
ETD-HIC 28 Rainer Fries
Application to the MV Model
Apply to the MV case At early times C = 0
Radial flow velocity at early times Assuming p = 1/3 e Independent of cutoff
tanhv
v
22
z
rr
r
rr
pA
V
pA
VpApe
22
21
22
21
2
3v
r
r
0rz
ETD-HIC 29 Rainer Fries
Space-Time Picture
Finally: field has decayed into plasma at = 0
Energy is taken from deceleration of the nuclei in the color field.
Full energy momentum conservation:
fTf
[Mishustin, Kapusta]
ETD-HIC 30 Rainer Fries
Space-Time Picture
Deceleration: obtain positions * and rapidities y* of the baryons at = 0
For given initial beam rapidity y0 , mass area density m.
BRAHMS: dy = 2.0 0.4 Nucleon: 100 GeV 27 GeV Rough estimate:
aavayy 121coshcosh 00*
m
fa 0
[Kapusta, Mishustin][Mishustin 2006]
20 GeV/fm 9f
ETD-HIC 31 Rainer Fries
Summary
Recursive solution for Yang Mills equations (boost-invariant case)
Strong initial longitudinal gluon fields
Negative longitudinal pressure baryon stopping
Transverse energy flow of energy starts at = 0
Use full energy momentum tensor to match to hydrodynamics
Constraining hydro initial conditions
ETD-HIC 32 Rainer Fries
Backup
ETD-HIC 33 Rainer Fries
Estimating Energy Density
Sum over contributions from all charges, recover continuum limit. Can be done analytically in simple situations In the following: center of head-on collision of very large
nuclei (RA >> Rc) with very slowly varying charge densities k (x) k.
E.g. initial energy density 0:
Depends logarithmically on ratio of scales = RcQ0.
2221
3
42.01ln c
sME N
[RJF, Kapusta, Li]
ETD-HIC 34 Rainer Fries
Energy Matching
Total energy content (soft plus pQCD) RHIC energy.