Pure double-layer bubbles in quadratic F (R) gravity

We present a class of spherically symmetric spacetimes corresponding to bubbles separating two regions with constant values of the scalar curvature, or equivalently with two different cosmological constants, in quadratic F(R) theory. The bubbles are obtained by means of the junction formalism, and t...

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Autores principales: Eiroa, E.F., Figueroa Aguirre, G., Senovilla, J.M.M.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_24700010_v95_n12_p_Eiroa
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spelling todo:paper_24700010_v95_n12_p_Eiroa2023-10-03T16:42:02Z Pure double-layer bubbles in quadratic F (R) gravity Eiroa, E.F. Figueroa Aguirre, G. Senovilla, J.M.M. We present a class of spherically symmetric spacetimes corresponding to bubbles separating two regions with constant values of the scalar curvature, or equivalently with two different cosmological constants, in quadratic F(R) theory. The bubbles are obtained by means of the junction formalism, and the matching hypersurface supports in general a thin shell and a gravitational double layer. In particular, we find that pure double layers are possible for appropriate values of the parameters of the model whenever the quadratic coefficient is negative. This is the first example of a pure double layer in a gravitational theory. © 2017 American Physical Society. Fil:Eiroa, E.F. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_24700010_v95_n12_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 We present a class of spherically symmetric spacetimes corresponding to bubbles separating two regions with constant values of the scalar curvature, or equivalently with two different cosmological constants, in quadratic F(R) theory. The bubbles are obtained by means of the junction formalism, and the matching hypersurface supports in general a thin shell and a gravitational double layer. In particular, we find that pure double layers are possible for appropriate values of the parameters of the model whenever the quadratic coefficient is negative. This is the first example of a pure double layer in a gravitational theory. © 2017 American Physical Society.
format JOUR
author Eiroa, E.F.
Figueroa Aguirre, G.
Senovilla, J.M.M.
spellingShingle Eiroa, E.F.
Figueroa Aguirre, G.
Senovilla, J.M.M.
Pure double-layer bubbles in quadratic F (R) gravity
author_facet Eiroa, E.F.
Figueroa Aguirre, G.
Senovilla, J.M.M.
author_sort Eiroa, E.F.
title Pure double-layer bubbles in quadratic F (R) gravity
title_short Pure double-layer bubbles in quadratic F (R) gravity
title_full Pure double-layer bubbles in quadratic F (R) gravity
title_fullStr Pure double-layer bubbles in quadratic F (R) gravity
title_full_unstemmed Pure double-layer bubbles in quadratic F (R) gravity
title_sort pure double-layer bubbles in quadratic f (r) gravity
url http://hdl.handle.net/20.500.12110/paper_24700010_v95_n12_p_Eiroa
work_keys_str_mv AT eiroaef puredoublelayerbubblesinquadraticfrgravity
AT figueroaaguirreg puredoublelayerbubblesinquadraticfrgravity
AT senovillajmm puredoublelayerbubblesinquadraticfrgravity
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