7.4. GALAXIES 447
galaxy nucleus
Figure 7.7: A schematic diagram of elliptical galaxy.
The metric is as in (7.4.3), and the corresponding fluid equations (7.1.65)-(7.1.68) are in
the form:
(7.4.7)
∂P
∂ τ
+
1
ρ
(P·∇)P=ν∆P−∇p−ρ( 1 −βT)
M 0 G
αr^2
~k,
∂T
∂ τ
+
1
ρ
(P·∇)T=κ∆ ̃T+Q,
∂ ρ
∂ τ
+divP= 0 ,
supplemented with the physically sound conditions:
(7.4.8)
Pr= 0 ,
∂Pθ
∂r
= 0 ,
∂Pφ
∂r
=0 atr=r 0 ,r 1 ,
T(r 0 ) =T 0 , T(r 1 ) =T 1.
3.Galaxy dynamics.Based on both models (7.4.4)-(7.4.5) and (7.4.7)-(7.4.8), we outline
below the large scale dynamics of both spiral and ellipticalgalaxies.
Let the models be abstractly written in the following form
(7.4.9)
du
dt
=F(u,ρ),
whereu= (P,T,p)is the unknown function, andρis the initial density distribution, which is
used as a control parameter representing different physical conditions.
First, we consider the stationary equation of (7.4.9) given by
(7.4.10) F(u,ρ) = 0.
Letu 0 be a solution of (7.4.10), and consider the deviation fromu 0 as
u=v+u 0.
Thus, (7.4.9) becomes the following form
(7.4.11)
dv
dt
=Lλv+G(v,λ,ρ),