Thermodynamics and Shadows of quantum-corrected Reissner-Nordstrom black hole surrounded by quintessence

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F62690094%3A18470%2F23%3A50020600" target="_blank" >RIV/62690094:18470/23:50020600 - isvavai.cz</a>

Výsledek na webu

<a href="http://dx.doi.org/10.1016/j.dark.2023.101293" target="_blank" >http://dx.doi.org/10.1016/j.dark.2023.101293</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1016/j.dark.2023.101293" target="_blank" >10.1016/j.dark.2023.101293</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Thermodynamics and Shadows of quantum-corrected Reissner-Nordstrom black hole surrounded by quintessence

Popis výsledku v původním jazyce

In this work, we consider the quantum-corrected Reissner-Nordstrom black hole surrounded by quintessence matter and examine its thermodynamics and shadow. To this end, we handle the quantum-corrected metric of the black hole, which is given by Wu and Lui in 2022, and couple the quintessence matter field effects to the lapse function. Then, we obtain the mass, Hawking temperature, specific heat, and equation of state functions. In all these functions, we discuss two cases in which the quantum corrections are greater or smaller than the quintessence matter effects. We observe that within these two scenarios, the black hole has different characteristic thermal behaviors. Moreover, we find that the quintessence matter plays an important role in leading to a black hole remnant. Furthermore, we observe that black hole behaves like Van der Waals fluid. Finally, we investigate the black hole shadow by Carter&apos;s approach. We find that quintessence matter and quantum corrections modify the shadow of the black hole.&amp; COPY; 2023 Elsevier B.V. All rights reserved.

Název v anglickém jazyce

Thermodynamics and Shadows of quantum-corrected Reissner-Nordstrom black hole surrounded by quintessence

Popis výsledku anglicky

In this work, we consider the quantum-corrected Reissner-Nordstrom black hole surrounded by quintessence matter and examine its thermodynamics and shadow. To this end, we handle the quantum-corrected metric of the black hole, which is given by Wu and Lui in 2022, and couple the quintessence matter field effects to the lapse function. Then, we obtain the mass, Hawking temperature, specific heat, and equation of state functions. In all these functions, we discuss two cases in which the quantum corrections are greater or smaller than the quintessence matter effects. We observe that within these two scenarios, the black hole has different characteristic thermal behaviors. Moreover, we find that the quintessence matter plays an important role in leading to a black hole remnant. Furthermore, we observe that black hole behaves like Van der Waals fluid. Finally, we investigate the black hole shadow by Carter&apos;s approach. We find that quintessence matter and quantum corrections modify the shadow of the black hole.&amp; COPY; 2023 Elsevier B.V. All rights reserved.

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

2023

Kód důvěrnosti údajů

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

Název periodika

PHYSICS OF THE DARK UNIVERSE

ISSN

2212-6864

e-ISSN

2212-6864

Svazek periodika

42

Číslo periodika v rámci svazku

December

Stát vydavatele periodika

NL - Nizozemsko

Počet stran výsledku

11

Strana od-do

"Article Number: 101293"

Kód UT WoS článku

001048310200001

EID výsledku v databázi Scopus

2-s2.0-85165560623