Thin shells surrounding black holes in F(R) gravity

In this article, we consider spherical thin shells of matter surrounding black holes in F(R) theories of gravity. We study the stability of the static configurations under perturbations that conserve the symmetry. In particular, we analyze the case of charged shells outside the horizon of non-charge...

Descripción completa

Guardado en:
Detalles Bibliográficos
Publicado: 2019
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14346044_v79_n2_p_Eiroa
http://hdl.handle.net/20.500.12110/paper_14346044_v79_n2_p_Eiroa
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_14346044_v79_n2_p_Eiroa
record_format dspace
spelling paper:paper_14346044_v79_n2_p_Eiroa2023-06-08T16:15:27Z Thin shells surrounding black holes in F(R) gravity In this article, we consider spherical thin shells of matter surrounding black holes in F(R) theories of gravity. We study the stability of the static configurations under perturbations that conserve the symmetry. In particular, we analyze the case of charged shells outside the horizon of non-charged black holes. We obtain that stable static thin shells are possible if the values of the parameters of the model are properly selected. © 2019, The Author(s). 2019 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14346044_v79_n2_p_Eiroa http://hdl.handle.net/20.500.12110/paper_14346044_v79_n2_p_Eiroa
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description In this article, we consider spherical thin shells of matter surrounding black holes in F(R) theories of gravity. We study the stability of the static configurations under perturbations that conserve the symmetry. In particular, we analyze the case of charged shells outside the horizon of non-charged black holes. We obtain that stable static thin shells are possible if the values of the parameters of the model are properly selected. © 2019, The Author(s).
title Thin shells surrounding black holes in F(R) gravity
spellingShingle Thin shells surrounding black holes in F(R) gravity
title_short Thin shells surrounding black holes in F(R) gravity
title_full Thin shells surrounding black holes in F(R) gravity
title_fullStr Thin shells surrounding black holes in F(R) gravity
title_full_unstemmed Thin shells surrounding black holes in F(R) gravity
title_sort thin shells surrounding black holes in f(r) gravity
publishDate 2019
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14346044_v79_n2_p_Eiroa
http://hdl.handle.net/20.500.12110/paper_14346044_v79_n2_p_Eiroa
_version_ 1768542097435000832

Ejemplares similares