4D scale-dependent Schwarzschild-AdS/dS black holes: study of shadow and weak deflection angle and greybody bounding

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Título: 4D scale-dependent Schwarzschild-AdS/dS black holes: study of shadow and weak deflection angle and greybody bounding
Autor/es: Övgün, Ali | Pantig, Reggie C. | Rincón, Ángel
Grupo/s de investigación o GITE: Astrofísica Relativista
Centro, Departamento o Servicio: Universidad de Alicante. Departamento de Física Aplicada
Palabras clave: Black holes | Schwarzschild-AdS/dS | Scale-dependent gravity | Shadow | Deflection angle | Greybody bounding
Fecha de publicación: 2-mar-2023
Editor: Springer Nature
Cita bibliográfica: The European Physical Journal Plus. 2023, 138:192. https://doi.org/10.1140/epjp/s13360-023-03793-w
Resumen: We investigate the shadow, deflection angle, and the greybody bounding of a Schwarzschild-AdS/dS black hole in scale-dependent gravity. We used the EHT data to constrain the parameter ϵ. We have found that within the 1σ level of uncertainty, ϵM0 ranges at 10−11 − 10−16 orders of magnitude for Sgr. A*, and 10−11 − 10−17 for M87*. Using these parameters, we explored how the shadow radius behaves as perceived by a static observer. Using the known parameters for Sgr. A* and M87*, we found different shadow cast behavior near the cosmological horizon even if the same scaling parameters were used. We explored the deflection angle ^α in the weak field limit for both massive and null particles, in addition to the effect of finite distances using the non-asymptotically flat version of the Gauss-Bonnet theorem. We have found that the ^α strongly depends on massive particles. Tests on ϵ’s effect using Sgr. A* is only along points of low impact parameters. For M87*, only the scaled BH in AdS type can be tested at high impact parameters at the expense of very low value for ^α. We study the rigorous bound on the greybody factor for scalar field emitted from black holes in the theory and show the bound on the transmission probability. The effects of the scale-dependent gravity on the greybody factors are investigated, and the results indicate that the bound on the greybody factor in this case is less than the bound for the Schwarzschild black hole.
Patrocinador/es: Open Access funding provided thanks to the CRUE-CSIC agreement with Springer Nature. A.R. is funded by the María Zambrano contract ZAMBRANO 21-25 (Spain). A. Ö. and R. P. would like to acknowledge networking support by the COST Action CA18108 - Quantum gravity phenomenology in the multi-messenger approach (QG-MM).
URI: http://hdl.handle.net/10045/132478
ISSN: 2190-5444
DOI: 10.1140/epjp/s13360-023-03793-w
Idioma: eng
Tipo: info:eu-repo/semantics/article
Derechos: © The Author(s) 2023. Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
Revisión científica: si
Versión del editor: https://doi.org/10.1140/epjp/s13360-023-03793-w
Aparece en las colecciones:INV - Astrofísica Relativista - Artículos de Revistas

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