Stability of gravastars with exterior regular black holes
Mar 9, 202017 pages
Published in:
- Annals Phys. 415 (2020) 168124
- Published: Apr, 2020
e-Print:
- 2003.04893 [gr-qc]
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Abstract: (Elsevier)
This paper examines the stability of thin-shell gravastars in the context of regular spacetimes (Bardeen and Bardeen-de Sitter black holes). We apply cut and paste approach to construct gravastars through the matching of interior non-singular de Sitter geometry with exterior regular black hole. This model contains three regions, i.e., interior, thin-shell and exterior. The interior and exterior regions are connected at thin-shell. We investigate physical viability of the developed model by the energy conditions and explore its stability by using radial perturbation about the equilibrium shell radius. It is found that thin-shell gravastars show large stable regions for the Bardeen-de Sitter black hole as compared to the Bardeen black hole. It is concluded that stable regions exist near the formation of expected event horizon.Note:
- 17 pages, 5 figures
- Gravastars
- Israel thin-shell formalism
- Stability analysis
References(34)
Figures(16)
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