446 CHAPTER 7. ASTROPHYSICS AND COSMOLOGY
galaxy nucleus
galaxy disk
Figure 7.6: A schematic diagram of spiral galaxy.
for which the spherical coordinates reduce to the polar coordinate system(φ,r):
(7.4.2) (θ,φ,r) =
(π
2
,φ,r
)
for 0≤φ≤ 2 π, r 0 <r<r 1.
The metric satisfying the gravitational field equations (7.1.62) of the galaxy nucleus is the
Schwarzschild solution:
(7.4.3)
g 00 =−
(
1 +
2
c^2
ψ
)
, ψ=−
M 0 G
r
,
g 11 =α(r) =
(
1 −
δr 0
r
)− 1
, δ=
2 M 0 G
c^2 r 0
,
wherer 0 <r<r 1 andM 0 is the mass of galactic nucleus.
With (7.4.2) and (7.4.3), the 2D fluid equations (7.1.65)-(7.1.68) are written as
(7.4.4)
∂Pφ
∂ τ
+
1
ρ
(P·∇)Pφ=ν∆Pφ−
1
r
∂p
∂ φ
,
∂Pr
∂ τ
+
1
ρ
(P·∇)Pr=ν∆Pr−
1
α
∂p
∂r
−ρ( 1 −βT)
MrG
αr^2
,
∂T
∂ τ
+
1
ρ
(P·∇)T=κ ̃∆T+Q,
∂ ρ
∂ τ
+divP= 0 ,
supplemented with boundary conditions:
(7.4.5)
Pφ(r 0 ) =ζ 0 , Pr(r 0 ) = 0 , T(r 0 ) =T 0 ,
Pφ(r 1 ) =ζ 1 , Pr(r 1 ) = 0 , T(r 1 ) =T 1.
Hereαis as in (7.4.3), andMris the total mass in the ballBr.
2.Elliptical galaxies.Elliptical galaxies are spherically-shaped, defined in a spherical-
annular domain, as shown in Figure7.7:
(7.4.6) Ω={x∈R^3 |r 0 <|x|<r 1 }