Stability of Rotating Supermassive Stars in the Presence of a Dark Matter Background
Open Access
- 20 April 1998
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 497 (2) , 559-562
- https://doi.org/10.1086/305505
Abstract
The stability of supermassive stars embedded in hot dark matter is investigated on the basis of the energetic method. The stability effect of dark matter is compared with rotational stabilization, and preference for the latter factor is advocated.Keywords
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