Thermodynamics of the Reissner-Nordstrom black hole with quintessence matter on the EGUP framework

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F62690094%3A18470%2F22%3A50019287" target="_blank" >RIV/62690094:18470/22:50019287 - isvavai.cz</a>

Výsledek na webu

<a href="http://dx.doi.org/10.1016/j.physletb.2022.136994" target="_blank" >http://dx.doi.org/10.1016/j.physletb.2022.136994</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1016/j.physletb.2022.136994" target="_blank" >10.1016/j.physletb.2022.136994</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Thermodynamics of the Reissner-Nordstrom black hole with quintessence matter on the EGUP framework

Popis výsledku v původním jazyce

In this paper, we investigate the quantum correction on thermodynamics of the Reissner-Nordstrom black hole in the presence of the quintessence matter associated with dark energy. To this end, the modified Hawking temperature, heat capacity, and entropy functions of the black hole are derived. Investigation reveals that the modified uncertainty principles and normalization factor alpha restrict the lower bound value of horizon radius to affect the Hawking temperature and the parameter eta(0) has a non-negligible effect on the heat capacity threshold. Furthermore, the correction of entropy does not depend on the quintessence matter. It is also examined the equation of state associated with the pressure and the volume in this framework. In addition, we employ graphical methods to compare and discuss the findings within the generalized uncertainty principle (GUP) and extended uncertainty principle (EUP). (c) 2022 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP(3).

Název v anglickém jazyce

Thermodynamics of the Reissner-Nordstrom black hole with quintessence matter on the EGUP framework

Popis výsledku anglicky

In this paper, we investigate the quantum correction on thermodynamics of the Reissner-Nordstrom black hole in the presence of the quintessence matter associated with dark energy. To this end, the modified Hawking temperature, heat capacity, and entropy functions of the black hole are derived. Investigation reveals that the modified uncertainty principles and normalization factor alpha restrict the lower bound value of horizon radius to affect the Hawking temperature and the parameter eta(0) has a non-negligible effect on the heat capacity threshold. Furthermore, the correction of entropy does not depend on the quintessence matter. It is also examined the equation of state associated with the pressure and the volume in this framework. In addition, we employ graphical methods to compare and discuss the findings within the generalized uncertainty principle (GUP) and extended uncertainty principle (EUP). (c) 2022 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP(3).

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2022

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Physics letters B

ISSN

0370-2693

e-ISSN

1873-2445

Svazek periodika

827

Číslo periodika v rámci svazku

April

Stát vydavatele periodika

NL - Nizozemsko

Počet stran výsledku

10

Strana od-do

"Article Number: 136994"

Kód UT WoS článku

000820935000040

EID výsledku v databázi Scopus

2-s2.0-85125644502