relativistic hydrodynamics – stability and causality p. ván 1,2 and t. s. bíró 1 rmki, budapest...
TRANSCRIPT
Relativistic hydrodynamics – stability and causality
P. Ván1,2 and T. S. Bíró1
RMKI, Budapest1 and University of Bergen2
– Introduction– Causality – parabolic equations– Stability – Eckart problem– Separation of dissipative and nondissipative parts– Conclusions
Zimányi 75 Memorial Workshop’07, Budapest
Nonrelativistic Relativistic
Local equilibrium (1st) Fourier, Navier-Stokes Eckart
Beyond local equilibrium Cattaneo-Vernotte, Israel-Stewart,(2nd) gen. Navier-Stokes Müller-Ruggieri
Öttinger, Carter, etc..
Conceptual issues plaguing relativistic hydrodynamics:
Causality – first order is bad – acausalsecond order is good - causal
Stability – first order is bad – instablesecond order is good - stable
Introduction:
Causality hyperbolic or parabolic? (Fichera 1992, Kostädt and Liu 2000)
Well-posedness Speed of signal propagation
0),,,,(2 TTTtxFTCTBTA txttxtxx
Second order linear partial differential equation:
02(*) 22 ttxx CBA
Corresponding equation of characteristics:
i) Hyperbolic equation: two distinct families of real characteristicsParabolic equation: one family of real characteristicsElliptic equation: no real characteristics
Well-posedness: existence, unicity, continuous dependence on initial data.
A characteristic Cauchy problem of (1) is well posed. (initial data on the characteristic surface: ))()0,( xfxT
,0 TT xxt (1)
iii) The outer real characteristics that pass through a given point give its domain of influence .
),( 00 tx0
02)(
,0
~~4
2
~~2~~~~
Tc
v
c
vTv
TT
tttxxxxt
xxt
(1)
ii) (*) is transformation invariant ),(~~),,(~~ txtttxxx
t
x
t
x
?
0
cv
vtx
E.g.
)()0,(
,0
xxT
TT xxt
t
x
et
AtxT
4
2
2),(
-4 -2 2 4
0.25
0.5
0.75
1
1.25
1.5
1.75
2
Infinite speed of signal propagation?physics - mathematics
Hydrodynamic range of validity:ξ – mean free pathτ – collision time
TT
TT tx
,
More complicated equations, more spacetime dimensions, ….
Water at room temperature:
Fermi gas of light quarks at :
t
x
et
AtxT
4
2
2),(
Vcv max
s
m
cv
V
14max
cTs
mmT
c
vmc
cv
V
V
V
31max 10
-4 -2 2 4
0.25
0.5
0.75
1
1.25
1.5
1.75
2
,0 TT xxt
homogeneous equilibrium (thermodynamics = theory of stability of …)
linear and nonlinearlinear – necessary condition
Eckart theory:instable – due to heat conduction
Stability of what and in what sense?
scpc
T 3422
10)(
water
Israel-Stewart theory: strange condition
relaxation to the first order theory (Geroch 1995, Lindblom 1995)
1)(1 p ...),(),,( 1 aa
ea qqnsqns
...),(),,,( 21 ababa
ae
aba qqnsqns
0 aa
aa
aa JussS
...1 T
q
T
qJ b
abaa
.....
0)( aaa
aa
aab
ba uqqupTu
Irreversible thermodynamics (standard method, e.g. B. Lukács):
Structure of dissipative hydrodynamic theories:
0)()(1
2 aa
a
ababab
aa
s uTTT
qupP
TTj
Eckart term
Complete Eckart system
.2
,
,
,
,0)(
,0
,0
ab
a
bv
cc
a
av
caca
ccaca
acbb
cac
ab
bbb
aacbb
ac
abab
aaa
aa
aab
ba
aa
aa
aa
uP
uP
Tj
uTTq
PquququT
uPuqquTu
junnN
.0,,,.,,, a
bvaaa Pqjconstun Equilibrium:
< > - symmetric traceless spacelike part
x
x
x
nn
en
en
j
q
u
n
ik
Tik
Tik
TTTikTik
ikppikpik
ikpik
ikikn
~1
0000
01
00
00
0)(
00)(0
000
2
Q
xy
y
y
q
u
ik
T
ikp
10
01
)(
R
0)()det( 22 kpTT R
Stability condition for transverse modes:
)exp(0 ikxtAA exponential plane-waves (Hiscock and Lindblom, 1985)
/4/3~
root with a positive real part instabilitycoupling of shear viscosity and heat conduction
Landau frame? aaq 0
First or second (or higher) order theory?
Causality: speed of the VALIDITY < speed of light both for first and second order
Stability: Landau choice (q=0) is a temporary escape - entropy production, multicomponent fluidsboth for first and second order
Origin of stability problem: wrong separation of dissipative and non dissipative terms and
effects
e.g. the choice of velocity field is not free (e.g. entropy production)
.0)ˆ(ˆ
,0ˆ
,0
acbb
cac
ab
bbb
aacbb
ac
abab
aaa
aa
aab
ba
aabb
PquququT
uPuqquTu
T
Separation condition:
0ˆ,ˆˆˆ aa
aaa ququeE
ababab
bab uquueuE 0)ˆˆ()ˆ(
Separation of dissipation (PV and TSB arXiv:0704.2039)
flow energy
ijj
iab
aba
aa
abbababaab
Pq
qeeT
PuquPuqquuuT
ˆ
ˆ
0,0,ˆ
Something more…
.0ˆˆˆˆ)(
,0ˆˆˆˆ)(aab
baca
cbc
bac
aaa
aba
ba
ueuqquEb
uqueeuEua
0ˆˆ bb
aa uEE.
(a) energies: total= internal+ flow (mass?)(b) velocity – momentum (heat) flow energy – heat flux
ababab
bb
aabab uquueuEEuE 0)ˆˆ(ˆˆ)ˆ(
0ˆ0,0 euq aa
Thermodynamics:
,ˆ,)ˆ( pTsEeTdsEed aa
Statics:
TE
s
e
sa
1ˆ
)(ˆ2
1ˆˆˆˆ 42222 qqq O
eeeqqeE a
aa
q dependence:
normal with internal energy e, or:
...ˆ2
1)()
ˆ2
1ˆ()ˆ( 22 qq
eTs
eeesEes a
Summary
– momentum density = but ≡ heat flow – energy = internal energy + flow energy
ADDS:– entropy flux and can ben justified
(thermodynamic theory construction – Liu procedure)
– linear stability of homogeneous equilibrium
Thermodynamics stability of matter
)ˆ( aEes
Thank you for your attention!
0)(
11
11)(
1
))((1
2
aa
a
aa
aa
a
aa
aa
aa
a
a
aa
aa
aa
aa
a
a
aa
a
aa
aa
aa
uTTT
q
Tquq
T
T
qqu
Tq
TuTsp
T
T
qusququp
T
T
qus
s
JussS
))(( aaa
aa
a uqqup
Tdsd
T
qJ
aa
pTs 0aaqu
01
1)(
1
))((1
)(
2
.
TT
q
Tq
T
TuTsEep
T
T
qusquEpe
T
T
qusE
E
se
e
s
JusEesS
a
a
aa
a
aa
aa
a
a
aa
aa
aa
a
a
aa
a
aa
aa
aa
TdsEed )(
pTsEe
.0)(
,0)(a
baba
bbacb
bac
aa
aa
abb
a
puqupeT
qupeeTu
Net balances:
....
....
,Tq caca
Balance of entropy:
Stable!
0)(1
2 T
T
qupP
TTj a
a
ababab
aa
0ˆ bab
abb uET
aaa
aaaean
aaean
aa
aaaaean
aa
aa
aa
aa
jquen
quTT
eTT
nTT
jeT
nT
u
queepnp
qupee
junn
.0
,0
,0
,0
,0)(
,0
222
LinearizationAAA 0
Routh-Hurwitz:
0)(
0,0
n
pnpe
e
pTne
T thermodynamic stability
hydrodynamic stability
TT
TTk
pTpTnT
pT
ppeTk
TT
TTpek
TTTkpnpepTk
TTTepTk
peT
QDet
enne
enneenne
enne
nene
ne
2
24
2
2222
2222
23
)(
)(
))((
))((
)(
)(
Nonrelativistic experience – a four vector formalism
Energy units of mass: )1(][][ ce
,0)3(
,0)2(
,0)1(
ijiji
ii
i
iijj
i
ii
vPqvee
Pv
v
mass
velocity (momentum ?)
internal energy
velocity-momentum (relativistic?).)4( ii vq
,0)2(
0:)4()2()1(iij
jj
jii
ijj
jj
ii
Pvqqa
Pvvv
,0)4( iijj
ii vvqqa
,0)3( ijiji
ii
i vPqvee ,0)2( iijj
jj
ii Pvqqa
AAvAAv
Au
uqqvu
xtx
ii
titibb
aaia
Tia
aia
),(1
1);,0(;),1(
);0,0,0,1();,(
spacelike, timelike, vectors and covectors,
substantial time derivative
,0~
aa
baab
abb
bab
baab
ab uqqPqveeT
Nonrelativistic spacetime: there is time (absolute)
j
jb
a
iP
qeT
0~
?energy-momentum tensor
0)1( iiv ,0)4( iij
jii vvqqa
0
)(
ab
baab
baa
baab
bab
uuqquuu
uquuE
aaa quE
mass-momentum vector
j
i
jb
ab
ab
a
iPq
qeuETT
~
)4()3()2()1(0)(0 aauEandT bab
bab
total energy-momentum tensor
separation of dissipative and nondissiaptive parts