Thermodynamical properties of a deformed Schwarzschild black hole via Dunkl generalization

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F62690094%3A18470%2F25%3A50022544" target="_blank" >RIV/62690094:18470/25:50022544 - isvavai.cz</a>

Výsledek na webu

<a href="https://www.worldscientific.com/doi/10.1142/S0217751X25500198" target="_blank" >https://www.worldscientific.com/doi/10.1142/S0217751X25500198</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1142/S0217751X25500198" target="_blank" >10.1142/S0217751X25500198</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Thermodynamical properties of a deformed Schwarzschild black hole via Dunkl generalization

Popis výsledku v původním jazyce

In this paper, we construct a deformed Schwarzschild black hole from the de Sitter gauge theory of gravity within Dunkl generalization and we determine the metric coefficients versus Dunkl parameter and parity operators. Since the spacetime coordinates are not affected by the group transformations, only fields are allowed to change under the action of the symmetry group. A particular ansatz for the gauge fields is chosen and the components of the strength tensor are computed as well. Additionally, we analyze the modifications on the thermodynamic properties to a spherically symmetric black hole due to Dunkl parameters for even and odd parities. Finally, we verify a novel remark highlighted from heat capacity: the appearance of a phase transition when the odd parity is taken into account.

Název v anglickém jazyce

Thermodynamical properties of a deformed Schwarzschild black hole via Dunkl generalization

Popis výsledku anglicky

In this paper, we construct a deformed Schwarzschild black hole from the de Sitter gauge theory of gravity within Dunkl generalization and we determine the metric coefficients versus Dunkl parameter and parity operators. Since the spacetime coordinates are not affected by the group transformations, only fields are allowed to change under the action of the symmetry group. A particular ansatz for the gauge fields is chosen and the components of the strength tensor are computed as well. Additionally, we analyze the modifications on the thermodynamic properties to a spherically symmetric black hole due to Dunkl parameters for even and odd parities. Finally, we verify a novel remark highlighted from heat capacity: the appearance of a phase transition when the odd parity is taken into account.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2025

Kód důvěrnosti údajů

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

Název periodika

International Journal of Modern Physics A

ISSN

0217-751X

e-ISSN

1793-656X

Svazek periodika

40

Číslo periodika v rámci svazku

07

Stát vydavatele periodika

SG - Singapurská republika

Počet stran výsledku

15

Strana od-do

"Article Number: 2550019"

Kód UT WoS článku

001453631700004

EID výsledku v databázi Scopus

2-s2.0-86000438353