viscous hydrodynamics and the qcd equation of state
DESCRIPTION
Viscous hydrodynamics and the QCD equation of state. Azwinndini Muronga 1,2 1 Centre for Theoretical Physics and Astrophysics Department of Physics, University of Cape Town, South Africa 2 UCT-CERN Research Centre Department of Physics, University of Cape Town, South Africa - PowerPoint PPT PresentationTRANSCRIPT
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Viscous hydrodynamics and the QCD equation of state
Azwinndini Muronga 1,2
1 Centre for Theoretical Physics and AstrophysicsDepartment of Physics, University of Cape
Town, South Africa2 UCT-CERN Research Centre
Department of Physics, University of Cape Town, South Africa
Workshop on “Hydrodynamics in Heavy Ion Collisions and QCD Equation of State”
April 21-22, 2008 : BNL, Long Island, NY, USA
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References
• Literature: AM, AM and D.H. Rischke, D. Teaney; U. Heinz et al; T. Koide et al., P. Romatschke et al, …
• Recall talks by P. Huovinen, M. Asakawa, C. Nonaka, T. Hirano, T.
Csorgo, • See also talks byT. Koide, T. Kodama, K. Dusling, H. Song, R. Fries,
P. Huovinen, N. Demir, A. l and Z. Xu Or come to the 10 days workshop program on
“Viscous Hydrodynamics and Transport Models”
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Numerical and Conceptual Questions for Dissipative Relativistic Fluid Dynamics
What is the underlying theory? What are the initial conditions? What are the boundary
conditions? What is the underlying equation of
state? What are the transport
coefficients? Which numerical algorithm is
implemented?
Which tests are caried out? Numerical viscosity? What are the additional
parameters? How is the freeze out
implemented?
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Where
0=∂∂
+∂∂
+∂∂
+∂∂
z
H
y
G
x
F
t
U
,
⎥⎥⎥⎥⎥⎥⎥
⎦
⎤
⎢⎢⎢⎢⎢⎢⎢
⎣
⎡
≡
E
M
M
M
N
Uz
y
x
( )
'
⎥⎥⎥⎥⎥⎥⎥
⎦
⎤
⎢⎢⎢⎢⎢⎢⎢
⎣
⎡
+π+π+π+∏++
π+
π+
π+∏++
≡
xz
zxy
yxx
xx
xzx
z
xyx
y
xxx
x
x
qvvvpE
vM
vM
pvM
Nv
F
( )
'
⎥⎥⎥⎥⎥⎥⎥
⎦
⎤
⎢⎢⎢⎢⎢⎢⎢
⎣
⎡
+π+π+π+∏++
π+
π+∏++
π+
≡
yz
zyx
xyy
yy
yzy
z
yyy
y
yxy
x
y
qvvvpE
vM
pvM
vM
Nv
G
( )
'
⎥⎥⎥⎥⎥⎥⎥
⎦
⎤
⎢⎢⎢⎢⎢⎢⎢
⎣
⎡
+π+π+π+∏++
π+∏++
π+
π+
≡
zy
yzx
xzz
zz
zzz
z
zyz
y
zxz
x
z
qvvvpE
pvM
vM
vM
Nv
H
Non-Relativistic dissipative fluid dynamics equations
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• The equations of fluid dynamics
( ) SUFUt =•∇+∂
,
⎥⎥⎥⎥⎥⎥⎥⎥
⎦
⎤
⎢⎢⎢⎢⎢⎢⎢⎢
⎣
⎡
π
∏=
q
M
E
N
U ( )( )( ) ( )( )
( ) ( )( )( ) ( )
⎥⎥⎥⎥⎥⎥⎥⎥
⎦
⎤
⎢⎢⎢⎢⎢⎢⎢⎢
⎣
⎡
⊗π⊗
∏⊗•π−π+⊗•−⊗γ+∏+−⊗
••π−•π+•−γ+∏++γ
=
v
vq
v
vvvvvqqvgpvM
vvvvvvqqvpE
v
UF
)(
Relativistic dissipative fluid dynamics equations
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( )
( )( )
⎥⎥⎥⎥⎥⎥⎥⎥⎥⎥⎥
⎦
⎤
⎢⎢⎢⎢⎢⎢⎢⎢⎢⎢⎢
⎣
⎡
θπ+π−πγτ
θ+−γτ
θ∏+∏−∏γτ=
π
∏
1
1
10
0
0
E
Eq
E
qqq
S
( )ση=π
+∇•−∂γκ−=
Θζ−=∏
2
, lnln
, 2
E
tE
E
aThTvTq
{ }{ } { }
vvghv
hvav
vvva
v
t
t
⊗γ−≡•∇=θ
Θ−⎭⎬⎫
⎩⎨⎧ γ⊗+γ⊗∇=σ
γ∇•γ+γ∂γ=
γ•∇+γ∂=Θ
2
)(
)(
,
, 3
1
2
1
,
,
Relativistic dissipative fluid dynamics equations
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αμα
μ
αβνβ
μα
μν
Λ=
πΛΛ=π
,
Calculational frame vs local rest frame of the fluid
( ) ( )( ) ( )( )( ) ( )( )( ) ( ) ,
,
vvvvvqqvgpvMP
vvvvvvqqvpEM
⊗•π−π+⊗•−⊗γ+∏+−⊗=
••π−•π+•−γ+∏++=
( )( ) . 1
, 1
Nvvn
vqvvME
•−=
•⎟⎠⎞⎜
⎝⎛ •−+−=ε
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Entropy 4-current, density and flux
Entropy 4-current
Entropy density
Entropy flux
Second Law of thermodynamics
The 3 new coefficients in the entropy density are related to the relaxation times and are responsible for causality while the 2 new coefficients in the entropy flux are related to the relaxation length and are responsible for the coupling between heat flow and viscous stresses
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Relaxation equations for dissipative fluxes
Relaxation equations for the dissipative fluxes
Transport and relaxation times/lengths
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Relaxation Coefficients
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Entropy density and entropy production
Entropy density
Entropy production
Relevant ratios ( )( )
( )( )ns
qn
ns
qns
eqeq ,
,,,,1
,
,,,,
ε
πΠεΨ−=
ε
πΠε νλν
Θ⎟⎠
⎞⎜⎝
⎛ΘΦ
−−= ss
s 1D
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Shear viscosity in the scaling solution
Energy equation
Reynold’s number vs eta/s
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Time evolution of thermodynamic quantities
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QCD EoS
Entropy equation of state
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Time evolution of thermodynamic quantities
QuickTime™ and a decompressor
are needed to see this picture.
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Time evolution of thermodynamic quantities
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Beyond the idealistic view of space-time evolution of relativistic heavy ion collisions
This talk discussed the intriguing questions of the non-equilibrium fluid dynamical description of the space-time evolution of the relativistic heavy
ion collisions. This description is quite different from the equilibrium description that we have learned to accept as the one that works.
It would be interesting to explore new non-equilibrium phenomena by combining the knowledge of non-
equilibrium relativistic fluid dynamics and relativistic kinetic/transport theory in the description of the space-
time evolution of relativistic heavy ion collisions.