Stability of Dynamically Collapsing Gas Sphere

preprint1999arXivOpen access

Abstract

We discuss stability of dynamically collapsing gas spheres. We use a similarity solution for a dynamically collapsing sphere as the unperturbed state. In the similarity solution the gas pressure is approximated by a polytrope of P=Kργ P = K ρ^γ. We examine three types of perturbations: bar (ℓ=2 \ell = 2) mode, spin-up mode, and Ori-Piran mode. When γ<1.097 γ< 1.097 , it is unstable against bar-mode. It is unstable against spin-up mode for any γ γ. When γ<0.961 γ< 0.961 , the similarity solution is unstable against Ori-Piran mode. The unstable mode grows in proportion to ∣t−t0∣−σ | t - t_0 | ^{-σ} while the central density increases in proportion to ρc∝(t−t0)−2 ρ_c \propto (t - t_0) ^{-2} in the similarity solution. The growth rate, σ σ is obtained numerically as a function of γ γ for bar mode and Ori-Piran mode. The growth rate of the bar mode is larger for a smaller γ γ. The spin-up mode has the growth rate of σ=1/3 σ= 1/3 for any γ γ.

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