Radiating Gravastars
Sep, 2011
Citations per year
Abstract: (arXiv)
Considering a Vaidya exterior spacetime, we study dynamical models of prototype gravastars, made of an infinitely thin spherical shell of a perfect fluid with the equation of state , enclosing an interior de Sitter spacetime. We show explicitly that the final output can be a black hole, an unstable gravastar, a stable gravastar or a 'bounded excursion' gravastar, depending on how the mass of the shell evolves in time, the cosmological constant and the initial position of the dynamical shell. This work presents, for the first time in the literature, a gravastar that emits radiation.Note:
- 23 pages and 17 figures, some typos corrected. Accepted for publication in JCAP
- 04.70.Dy
- 98.80.-k
- 04.20.Cv
- gravastar: stability
- space-time: de Sitter
- space-time: Vaidya
- radiation: emission
- gravastar
- equation of state
References(27)
Figures(23)