Gravitational Collapse and Singularity Removal in Rastall Theory

In the present work, we study spherically symmetric gravitational collapse of a homogeneous fluid in the framework of Rastall gravity. Considering a nonlinear equation of state (EoS) for the fluid profiles, we search for a class of nonsingular collapse solutions and the possibility of singularity re...

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Main Author: Ehsan Dorrani
Format: Article
Language:English
Published: Wiley 2021-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2021/6638827
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author Ehsan Dorrani
author_facet Ehsan Dorrani
author_sort Ehsan Dorrani
collection DOAJ
description In the present work, we study spherically symmetric gravitational collapse of a homogeneous fluid in the framework of Rastall gravity. Considering a nonlinear equation of state (EoS) for the fluid profiles, we search for a class of nonsingular collapse solutions and the possibility of singularity removal. We find that depending on the model parameters, the collapse scenario halts at a minimum value of the scale factor at which a bounce occurs. The collapse process then enters an expanding phase in the postbounce regime, and consequently the formation of a spacetime singularity is prevented. We also find that, in comparison to the singular case where the apparent horizon forms to cover the singularity, the formation of apparent horizon can be delayed allowing thus the bounce to be causally connected to the external universe. The nonsingular solutions we obtain satisfy the weak energy condition (WEC) which is crucial for physical validity of the model.
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spelling doaj-art-0c9be398b4cc4e29ba1d90d39e685ca42025-02-03T06:43:28ZengWileyAdvances in High Energy Physics1687-73571687-73652021-01-01202110.1155/2021/66388276638827Gravitational Collapse and Singularity Removal in Rastall TheoryEhsan Dorrani0Department of Physics, Kahnooj Branch, Islamic Azad University, Kahnooj, IranIn the present work, we study spherically symmetric gravitational collapse of a homogeneous fluid in the framework of Rastall gravity. Considering a nonlinear equation of state (EoS) for the fluid profiles, we search for a class of nonsingular collapse solutions and the possibility of singularity removal. We find that depending on the model parameters, the collapse scenario halts at a minimum value of the scale factor at which a bounce occurs. The collapse process then enters an expanding phase in the postbounce regime, and consequently the formation of a spacetime singularity is prevented. We also find that, in comparison to the singular case where the apparent horizon forms to cover the singularity, the formation of apparent horizon can be delayed allowing thus the bounce to be causally connected to the external universe. The nonsingular solutions we obtain satisfy the weak energy condition (WEC) which is crucial for physical validity of the model.http://dx.doi.org/10.1155/2021/6638827
spellingShingle Ehsan Dorrani
Gravitational Collapse and Singularity Removal in Rastall Theory
Advances in High Energy Physics
title Gravitational Collapse and Singularity Removal in Rastall Theory
title_full Gravitational Collapse and Singularity Removal in Rastall Theory
title_fullStr Gravitational Collapse and Singularity Removal in Rastall Theory
title_full_unstemmed Gravitational Collapse and Singularity Removal in Rastall Theory
title_short Gravitational Collapse and Singularity Removal in Rastall Theory
title_sort gravitational collapse and singularity removal in rastall theory
url http://dx.doi.org/10.1155/2021/6638827
work_keys_str_mv AT ehsandorrani gravitationalcollapseandsingularityremovalinrastalltheory