Shadows, greybody factors, emission rate, topological charge, and phase transitions for a charged black hole with a Kalb-Ramond field background

Fuente: arXiv
Enregistré dans:
Détails bibliographiques
Auteurs principaux: Hosseinifar, F., Filho, A. A. Araújo, Zhang, M. Y., Chen, H., Hassanabadi, H.
Format: Preprint
Publié: 2024
Sujets:
Accès en ligne:
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
_version_ 1866911949477904384
author Hosseinifar, F.
Filho, A. A. Araújo
Zhang, M. Y.
Chen, H.
Hassanabadi, H.
author_facet Hosseinifar, F.
Filho, A. A. Araújo
Zhang, M. Y.
Chen, H.
Hassanabadi, H.
contents In this work, we investigate a spherically symmetric charged black hole in the presence of a Kalb--Ramond field background. We calculate the photon sphere and shadow radii and, corroborating our results, we constrain them from observational data from the Event Horizon Telescope (EHT), particularly focusing on the shadow images of Sagittarius $A^{*}$. Additionally, we analyze the greybody factors, emission rate, and partial absorption cross section. We also examine the topological charge and its application to the deflection angle. Finally, we conduct the analysis of the heat capacity and phase transitions.
format Preprint
id arxiv_https___arxiv_org_abs_2407_07017
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Shadows, greybody factors, emission rate, topological charge, and phase transitions for a charged black hole with a Kalb-Ramond field background
Hosseinifar, F.
Filho, A. A. Araújo
Zhang, M. Y.
Chen, H.
Hassanabadi, H.
General Relativity and Quantum Cosmology
High Energy Physics - Theory
In this work, we investigate a spherically symmetric charged black hole in the presence of a Kalb--Ramond field background. We calculate the photon sphere and shadow radii and, corroborating our results, we constrain them from observational data from the Event Horizon Telescope (EHT), particularly focusing on the shadow images of Sagittarius $A^{*}$. Additionally, we analyze the greybody factors, emission rate, and partial absorption cross section. We also examine the topological charge and its application to the deflection angle. Finally, we conduct the analysis of the heat capacity and phase transitions.
title Shadows, greybody factors, emission rate, topological charge, and phase transitions for a charged black hole with a Kalb-Ramond field background
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2407.07017