Thermodynamic product formulae for Finslerian Kiselev black hole

Abstract The main goal of this paper is to solve the Finslerian Kiselev black hole and investigate its thermodynamic characteristics surrounded by dust, radiation, quintessence, and the cosmological constant. Since these black holes have multiple horizons, thus we calculate thermodynamic quantities,...

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Main Authors: Z. Nekouee, S. K. Narasimhamurthy
Format: Article
Language:English
Published: SpringerOpen 2023-08-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-023-11898-w
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author Z. Nekouee
S. K. Narasimhamurthy
author_facet Z. Nekouee
S. K. Narasimhamurthy
author_sort Z. Nekouee
collection DOAJ
description Abstract The main goal of this paper is to solve the Finslerian Kiselev black hole and investigate its thermodynamic characteristics surrounded by dust, radiation, quintessence, and the cosmological constant. Since these black holes have multiple horizons, thus we calculate thermodynamic quantities, including area, horizon radius, Bekenstein–Hawking entropy, Hawking temperature, surface gravity, and Komar energy products. In addition, we study all universal relations of these black holes and discuss the role and effect of the Finslerian Ricci scalar $$(\eta )$$ ( η ) on Finslerian Kiselev black holes and their stability.
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spelling doaj.art-48d854cb94ca4b80b1320d2285e029242023-09-17T11:24:54ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522023-08-0183811210.1140/epjc/s10052-023-11898-wThermodynamic product formulae for Finslerian Kiselev black holeZ. Nekouee0S. K. Narasimhamurthy1Department of PG Studies and Research in Mathematics, Kuvempu UniversityDepartment of PG Studies and Research in Mathematics, Kuvempu UniversityAbstract The main goal of this paper is to solve the Finslerian Kiselev black hole and investigate its thermodynamic characteristics surrounded by dust, radiation, quintessence, and the cosmological constant. Since these black holes have multiple horizons, thus we calculate thermodynamic quantities, including area, horizon radius, Bekenstein–Hawking entropy, Hawking temperature, surface gravity, and Komar energy products. In addition, we study all universal relations of these black holes and discuss the role and effect of the Finslerian Ricci scalar $$(\eta )$$ ( η ) on Finslerian Kiselev black holes and their stability.https://doi.org/10.1140/epjc/s10052-023-11898-w
spellingShingle Z. Nekouee
S. K. Narasimhamurthy
Thermodynamic product formulae for Finslerian Kiselev black hole
European Physical Journal C: Particles and Fields
title Thermodynamic product formulae for Finslerian Kiselev black hole
title_full Thermodynamic product formulae for Finslerian Kiselev black hole
title_fullStr Thermodynamic product formulae for Finslerian Kiselev black hole
title_full_unstemmed Thermodynamic product formulae for Finslerian Kiselev black hole
title_short Thermodynamic product formulae for Finslerian Kiselev black hole
title_sort thermodynamic product formulae for finslerian kiselev black hole
url https://doi.org/10.1140/epjc/s10052-023-11898-w
work_keys_str_mv AT znekouee thermodynamicproductformulaeforfinsleriankiselevblackhole
AT sknarasimhamurthy thermodynamicproductformulaeforfinsleriankiselevblackhole