430 CHAPTER 7. ASTROPHYSICS AND COSMOLOGY
- When a very massive red giant completely consumes its central supply of nuclear fuels,
its core collapses. Its radiusr 0 begins to decrease, and consequently theδ-factor increases:
r 0 decreases⇒δ=
2 mG
c^2 r 0
increases.
- The huge massmand the rapidly reduced radiusr 0 make theδ-factor approaching one:
δ→1 asr 0 →Rs
whereRs= 2 mG/c^2 is the Schwarzschild radius.
- By (7.2.58), the shrinking of the star slows down:
Pr∼
√
1 −δ,
and nearly stops asδ→ 1.
4). Then the model (7.2.26) is valid, and the eigenvalue equations of (7.2.26) are given
by
(7.2.60)
Pr∆P+
1
κ
FGP+σT~k−∇p=βP,
̃∆T+Pr=βT,
divP= 0.
The first eigenvalueβdepends on theδ-factor, and by (7.2.14)
(7.2.61) β 1 ∼
(
Prδ^2
1 −δ
) 1 / 2
asδ→ 1.
Based on the transition criterion (7.2.25), the property (7.2.61) implies that the star has con-
vection in the shell layer, i.e., the radial circulation momentum fluxPrsatisfies
Pr>0 in certain regions of the shell layer.
- The radial force (7.2.15) in the shell layer is
fr≃
2 Prδ^2
1 −δ
Pr→∞ asδ→1 andPr> 0 ,
which provides a very riving force, resulting in the supernova explosion, as shown in Figure
7.2.
- SincePr=0 atr=r 0 , the radial force of (7.2.14) is zero:
fr=0 at r=r 0.
Herer 0 is the radius of the blackhole core. Hence, the supernova’s huge explosion preserves
an interior core of smaller radius containing the blackholecore, which yields a neutron star.