Перейти к основному содержанию
AkademIndex

Продукты

Для разработчиков

AkademBaseскороОткрытый API экосистемы
Статья

Thermodynamic topology of black holes in F(R)-Euler–Heisenberg gravity’s Rainbow

Yassine SekhmaniCenter for Theoretical Physics, Khazar University, 41 Mehseti Street, Baku AZ1096, AzerbaijanSaeed Noori GashtiSchool of Physics, Damghan University, P. O. Box 3671641167, Damghan, IranMohammad Ali S. AfsharCanadian Quantum Research Center, 204-3002 32 Ave Vernon, BC V1T 2L7, CanadaMohammad Reza AlipourSchool of Physics, Damghan University, P. O. Box 3671641167, Damghan, IranJ. SadeghiCanadian Quantum Research Center, 204-3002 32 Ave Vernon, BC V1T 2L7, CanadaB. PourhassanCenter for Theoretical Physics, Khazar University, 41 Mehseti Street, Baku, AZ1096, AzerbaijanS. K. MauryaDepartment of Mathematical and Physical Sciences, College of Arts and Sciences, University of Nizwa, P. O. Box 33, Nizwa 616, Sultanate of OmanJavlon RayimbaevNational University of Uzbekistan, Tashkent 100174, Uzbekistan
ABI

Аннотация

The topology of black hole thermodynamics is a fascinating area of study that explores the connections between thermodynamic properties and topological features of black holes. It often involves analyzing critical points in the phase diagrams of black holes and assigning topological charges to these points. One significant approach is based on Duan’s topological current [Formula: see text]-mapping theory, which introduces the concept of topological charges to critical points in black hole thermodynamics. We successfully derive the field equations for [Formula: see text]-Euler–Heisenberg theory, providing a framework for studying the interplay between modified gravity and nonlinear electromagnetic effects. We obtain an analytical solution for a static, spherically symmetric, energy-dependent black hole with constant scalar curvature. Also, our analysis of black holes in F(R)-Euler–Heisenberg gravity’s Rainbow reveals significant insights into their topological properties. We identified the total topological charges by examining the normalized field lines along various free parameters. Our findings indicate that the parameters [Formula: see text] and [Formula: see text] influence the topological charges. These results are comprehensively summarized in Tables. In examining the photon sphere within this model, the sign of the parameter [Formula: see text] plays a crucial role in determining whether the model adopts a dS or AdS configuration. An interesting characteristic of this model is that, in its AdS form, it avoids the formation of naked singularity regions, which sets it apart from many other models. Typically, varying parameter values in other models can result in the division of space into regions of black holes and naked singularities. However, this model consistently retains its black hole behavior by featuring an unstable photon sphere, regardless of parameter values within the acceptable range. In its dS form, the behavior of the model’s photon sphere remains consistent with other dS models and does not exhibit unique differences.

Перевод пока недоступен

Темы

Идентификаторы

Цитирования и источники

Цитирований: 1Использованных источников: 0
Показатели — AkademScholar · Скоро