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) space 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.
Keywords
Cite
@article{arxiv.1904.04660,
title = {Cylindrical symmetric, non-rotating and non-static or static black hole solutions and the naked singularities},
author = {Faizuddin Ahmed},
journal= {arXiv preprint arXiv:1904.04660},
year = {2019}
}
Comments
32 pages, 4 figures, typos corrected, accepted for the publication in European Physical Journal C. arXiv admin note: text overlap with arXiv:1811.01707; text overlap with arXiv:gr-qc/9609065 by other authors