Growth of a Vortex Mode during Gravitational Collapse Resulting in Type II Supernova

Details Growth of a Vortex Mode during Gravitational Collapse Resulting in Type II Supernova Growth of a Vortex Mode during Gravitational Collapse Resulting in Type II Supernova

2000-01-26

arxiv.org/abs/astro-ph/0001447v1

Astronomy and Astrophysics

Astrophysics

AAS LaTeX, 14 pages including 6 figures, submitted to Astrophysical Journal in January

Scientific paper

10.1086/309370

We investigate stability of a gravitationally collapsing iron core against non-spherical perturbation. The gravitationally collapsing iron core is approximated by a similarity solution for dynamically collapsing polytropic gas sphere. We find that the similarity solution is unstable against non-spherical perturbations. The perturbation grows in proportion to $ (t - t_0) ^{-\sigma} $ while the the central density increases in proportion to $ (t - t_0) ^{-2} $. The growth rate is $ \sigma = 1/3 + \ell (\gamma - 4/3) $, where $ \gamma $ and $ \ell $ denote the polytropic index and the parameter $ \ell $ of the spherical harmonics, $ Y_{\ell} ^m (\theta, \phi) $, respectively. The growing perturbation is dominated by vortex motion. Thus it excites global convection during the collapse and may contribute to material mixing in a type II supernova.

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