Mathematical Principles of Theoretical Physics

(Rick Simeone) #1

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

=Force,

whereτis the proper time given by


(7.1.64) dτ=



−g 00 dt,

Pis the momentum density field, formally defined by


dx

=


1


ρ

P,


withρbeing the energy density,


dP

=


∂P


∂ τ

+


∂P


∂xk

dxk

=


∂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:

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