Cylindrical symmetric, non-rotating and non-static or static black hole solutions and the naked singularities

Abstract In this work, a four-dimensional cylindrical symmetric and non-static or static space-times in the backgrounds of anti-de Sitter (AdS) spaces with perfect stiff fluid, anisotropic fluid and electromagnetic field as the stress–energy tensor, is presented. For suitable parameter conditions in...

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Main Author: Faizuddin Ahmed
Format: Article
Language:English
Published: SpringerOpen 2019-06-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-019-7017-8
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author Faizuddin Ahmed
author_facet Faizuddin Ahmed
author_sort Faizuddin Ahmed
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description Abstract In this work, a four-dimensional cylindrical symmetric and non-static or static space-times in the backgrounds of anti-de Sitter (AdS) spaces with perfect stiff fluid, anisotropic fluid and electromagnetic field as the stress–energy tensor, is presented. For suitable parameter conditions in the metric function, the solution represents non-static or static non-rotating black hole solution. In addition, we show for various parameter conditions, the solution represents static and/or non-static models with a naked singularity without an event horizon.
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spelling doaj.art-0acd1d8227a945078b850ccb5df8d57a2022-12-21T18:23:52ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522019-06-0179611110.1140/epjc/s10052-019-7017-8Cylindrical symmetric, non-rotating and non-static or static black hole solutions and the naked singularitiesFaizuddin Ahmed0Ajmal College of Arts and ScienceAbstract In this work, a four-dimensional cylindrical symmetric and non-static or static space-times in the backgrounds of anti-de Sitter (AdS) spaces with perfect stiff fluid, anisotropic fluid and electromagnetic field as the stress–energy tensor, is presented. For suitable parameter conditions in the metric function, the solution represents non-static or static non-rotating black hole solution. In addition, we show for various parameter conditions, the solution represents static and/or non-static models with a naked singularity without an event horizon.http://link.springer.com/article/10.1140/epjc/s10052-019-7017-8
spellingShingle Faizuddin Ahmed
Cylindrical symmetric, non-rotating and non-static or static black hole solutions and the naked singularities
European Physical Journal C: Particles and Fields
title Cylindrical symmetric, non-rotating and non-static or static black hole solutions and the naked singularities
title_full Cylindrical symmetric, non-rotating and non-static or static black hole solutions and the naked singularities
title_fullStr Cylindrical symmetric, non-rotating and non-static or static black hole solutions and the naked singularities
title_full_unstemmed Cylindrical symmetric, non-rotating and non-static or static black hole solutions and the naked singularities
title_short Cylindrical symmetric, non-rotating and non-static or static black hole solutions and the naked singularities
title_sort cylindrical symmetric non rotating and non static or static black hole solutions and the naked singularities
url http://link.springer.com/article/10.1140/epjc/s10052-019-7017-8
work_keys_str_mv AT faizuddinahmed cylindricalsymmetricnonrotatingandnonstaticorstaticblackholesolutionsandthenakedsingularities