Polymer Black Hole Surrounded by Quintessence

Fuente: arXiv
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Autores principales: Araújo, M. C., Lima, J. G., Muniz, C. R., Furtado, J.
Formato: Preprint
Publicado: 2025
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author Araújo, M. C.
Lima, J. G.
Muniz, C. R.
Furtado, J.
author_facet Araújo, M. C.
Lima, J. G.
Muniz, C. R.
Furtado, J.
contents In this paper, we study the polymer black hole solution surrounded by a quintessence field. The influence of quintessence on the polymer black hole is investigated through its thermodynamic properties, such as the Hawking temperature, entropy, and specific heat, which allow us to address the question of thermodynamic stability. We then calculate bounds on the electromagnetic greybody factors and photon emission rates of the black hole, highlighting the interplay between quintessence and quantum gravity effects in determining these phenomena. We also examine the effects of quintessence and quantum gravity on the geodesics and shadows of massless particles around the black hole. Our results are further compared with observational data of the Sagittarius A black hole from the Event Horizon Telescope (EHT) collaboration.
format Preprint
id arxiv_https___arxiv_org_abs_2507_07372
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Polymer Black Hole Surrounded by Quintessence
Araújo, M. C.
Lima, J. G.
Muniz, C. R.
Furtado, J.
General Relativity and Quantum Cosmology
In this paper, we study the polymer black hole solution surrounded by a quintessence field. The influence of quintessence on the polymer black hole is investigated through its thermodynamic properties, such as the Hawking temperature, entropy, and specific heat, which allow us to address the question of thermodynamic stability. We then calculate bounds on the electromagnetic greybody factors and photon emission rates of the black hole, highlighting the interplay between quintessence and quantum gravity effects in determining these phenomena. We also examine the effects of quintessence and quantum gravity on the geodesics and shadows of massless particles around the black hole. Our results are further compared with observational data of the Sagittarius A black hole from the Event Horizon Telescope (EHT) collaboration.
title Polymer Black Hole Surrounded by Quintessence
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2507.07372