Stability of rotating supermassive stars in presence of dark matter background

Abstract

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.

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

Cited by in corpus (6)

• Evolution of Rotating Supermassive Stars to the Onset of Collapse
• The Growth of the Stellar Seeds of Supermassive Black Holes
• General Relativistic Instability Supernova of a Supermassive Population III Star
• Maximally Rotating Supermassive Stars at the Onset of Collapse: The Perturbative Effects of Gas Pressure, Magnetic Fields, Dark Matter and Dark Energy
• General-relativistic instability in rapidly accreting supermassive stars in the presence of dark matter
• Dark Matter and General Relativistic Instability in Supermassive Stars