7.1. ASTROPHYSICAL FLUID DYNAMICS 407
whereAμis the electromagnetic potential, the time components ofgμ νare as
g 00 =−
(
1 +
2
c^2
ψ
)
, g 0 k=gk 0 = 0 for 1≤k≤ 3 ,
andψis the gravitational potential.
2.Fluid dynamic equations.The Newton Second Law can be expressed as
(7.1.63)
dP
dτ
=Force,
whereτis the proper time given by
(7.1.64) dτ=
√
−g 00 dt,
Pis the momentum density field, formally defined by
dx
dτ
=
1
ρ
P,
withρbeing the energy density,
dP
dτ
=
∂P
∂ τ
+
∂P
∂xk
dxk
dτ
=
∂P
∂ τ
+
1
ρ
(P·∇)P,
and
ν∆P+μ∇(divP) the frictional force,
−∇p the pressure gradient,
c^2
2
ρ( 1 −βT)∇g 00 =−ρ( 1 −βT)∇ψ the gravitational force.
Hence, the momentum form of the fluid dynamic equations (7.1.63) is written as
(7.1.65)
∂P
∂ τ
+
1
ρ
(P·∇)P=ν∆P+μ∇(divP)−∇p−ρ( 1 −βT)∇ψ,
where the differential operators∆,∇and(P·∇)are with respect to the space metricgij( 1 ≤
i,j≤ 3 )determined by (7.1.62), as defined in (7.1.2)-(7.1.8).
3.Heat conduction equation:
(7.1.66)
∂T
∂ τ
+
1
ρ
(P·∇)T=κ∆ ̃T+Q,
where ̃∆is defined as
̃∆T=−√^1
g
∂
∂xi
(
√
ggij
∂T
∂xj
),
andg=det(gij), 1 ≤i,j≤3.
4.Energy-momentum conservation:
(7.1.67)
∂ ρ
∂ τ
+divP= 0 ,
whereρis the energy density: