Stability of rotating supermassive stars in presence of dark matter background

Details Stability of rotating supermassive stars in presence of dark matter background Stability of rotating supermassive stars in presence of dark matter background

1997-12-24

arxiv.org/abs/astro-ph/9712323v1

Astronomy and Astrophysics

Astrophysics

11 pages, 1 figure. ApJ, 1998 (accepted)

Scientific paper

10.1086/305505

Stability of supermassive stars embedded in hot dark matter is investigated
on the base of the energetic method. Stability effect of dark mater is compared
with rotational stabilization and preference of the last factor is advocated.

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