Gravastar model in Randall-Sundrum braneworld

José D.V. Arbañil, Pedro H.R.S. Moraes, Manuel Malheiro

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

4 Citas (Scopus)

Resumen

In this work we derive a gravastar model in Randall-Sundrum II braneworld scenario. Gravastars (or gravitationally vacuum stars) were proposed by Mazur and Mottola as systems of gravitational collapse alternative to black holes. The external region of the gravastar is described by a Schwarzschild space-time, while its internal region is filled by dark energy. In between there is a thin shell surface with ultrarelativistic matter (sometimes referred to as stiff matter). We obtain solutions for some physical quantities of the braneworld gravastars. Those are compared to original Mazur-Mottola results as well as with some gravastar solutions in alternative gravity theories. The consequences of the braneworld setup in gravastar physics is deeply discussed.

Idioma originalInglés
Número de artículo235012
PublicaciónClassical and Quantum Gravity
Volumen36
N.º23
DOI
EstadoPublicada - 1 nov. 2019
Publicado de forma externa

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© 2019 IOP Publishing Ltd.

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