Tidal forces around Schwarzschild black hole in cloud of strings and quintessence

Abstract We study the tidal forces and their effect in Schwarzschild black hole surrounded with clouds of strings and quintessence. Two horizons are present for this black hole and the event horizon shrinks on increasing the values of both, the string cloud and quintessence parameters. Tidal forces...

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Main Author: Rashmi Uniyal
Format: Article
Language:English
Published: SpringerOpen 2022-06-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-022-10520-9
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author Rashmi Uniyal
author_facet Rashmi Uniyal
author_sort Rashmi Uniyal
collection DOAJ
description Abstract We study the tidal forces and their effect in Schwarzschild black hole surrounded with clouds of strings and quintessence. Two horizons are present for this black hole and the event horizon shrinks on increasing the values of both, the string cloud and quintessence parameters. Tidal forces in radial as well as angular directions are independent of string cloud parameter a. Geodesic deviation equations are devised and solved for this BH metric. For numerical representation of the solutions of geodesic deviation equations two different initial conditions have been applied. Results are compared with that of Schwarzschild black hole metric.
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spelling doaj.art-a7df3ef70f984b3cb08739d29e0551622022-12-22T02:27:56ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522022-06-018261810.1140/epjc/s10052-022-10520-9Tidal forces around Schwarzschild black hole in cloud of strings and quintessenceRashmi Uniyal0Department of Physics, Dharmanand Uniyal Government Degree CollegeAbstract We study the tidal forces and their effect in Schwarzschild black hole surrounded with clouds of strings and quintessence. Two horizons are present for this black hole and the event horizon shrinks on increasing the values of both, the string cloud and quintessence parameters. Tidal forces in radial as well as angular directions are independent of string cloud parameter a. Geodesic deviation equations are devised and solved for this BH metric. For numerical representation of the solutions of geodesic deviation equations two different initial conditions have been applied. Results are compared with that of Schwarzschild black hole metric.https://doi.org/10.1140/epjc/s10052-022-10520-9
spellingShingle Rashmi Uniyal
Tidal forces around Schwarzschild black hole in cloud of strings and quintessence
European Physical Journal C: Particles and Fields
title Tidal forces around Schwarzschild black hole in cloud of strings and quintessence
title_full Tidal forces around Schwarzschild black hole in cloud of strings and quintessence
title_fullStr Tidal forces around Schwarzschild black hole in cloud of strings and quintessence
title_full_unstemmed Tidal forces around Schwarzschild black hole in cloud of strings and quintessence
title_short Tidal forces around Schwarzschild black hole in cloud of strings and quintessence
title_sort tidal forces around schwarzschild black hole in cloud of strings and quintessence
url https://doi.org/10.1140/epjc/s10052-022-10520-9
work_keys_str_mv AT rashmiuniyal tidalforcesaroundschwarzschildblackholeincloudofstringsandquintessence