Black hole shadow in f(R) gravity with nonlinear electrodynamics
Autor(a) principal: | |
---|---|
Data de Publicação: | 2023 |
Outros Autores: | , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1088/1674-1137/aca4bc http://hdl.handle.net/11449/246636 |
Resumo: | By analyzing the propagation of discontinuity in nonlinear electrodynamics, we numerically investigate the related black hole shadows of recently derived rotating black hole solutions in gravity. In this context, the geodesic motion of the relevant perturbations is governed by an effective geometry, which is closely related to the underlying spacetime metric. We derive the effective geometry, and the latter is used to determine the trajectory of the propagation vector of an arbitrary finite discontinuity in the electrodynamic perturbations, namely, the photon. Subsequently, the image of the black hole is evaluated using the ray-tracing technique. Moreover, we discuss the physical relevance of metric parameters, such as the nonlinear coupling, spin, and charge, by studying their impact on the resultant black hole shadows. |
id |
UNSP_35ae7ae957719986576f5db499dec4a3 |
---|---|
oai_identifier_str |
oai:repositorio.unesp.br:11449/246636 |
network_acronym_str |
UNSP |
network_name_str |
Repositório Institucional da UNESP |
repository_id_str |
2946 |
spelling |
Black hole shadow in f(R) gravity with nonlinear electrodynamicsblack hole shadoweffective metricnonlinear electrodynamicsBy analyzing the propagation of discontinuity in nonlinear electrodynamics, we numerically investigate the related black hole shadows of recently derived rotating black hole solutions in gravity. In this context, the geodesic motion of the relevant perturbations is governed by an effective geometry, which is closely related to the underlying spacetime metric. We derive the effective geometry, and the latter is used to determine the trajectory of the propagation vector of an arbitrary finite discontinuity in the electrodynamic perturbations, namely, the photon. Subsequently, the image of the black hole is evaluated using the ray-tracing technique. Moreover, we discuss the physical relevance of metric parameters, such as the nonlinear coupling, spin, and charge, by studying their impact on the resultant black hole shadows.Center for Gravitation and Cosmology College of Physical Science and Technology Yangzhou UniversityEscola de Engenharia de Lorena Universidade de São Paulo, SPSchool of Aeronautics and Astronautics Shanghai Jiao Tong UniversityFaculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista, SPInstitute of Physics Department of Physics Hunan Normal University, HunanFaculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista, SPYangzhou UniversityUniversidade de São Paulo (USP)Shanghai Jiao Tong UniversityUniversidade Estadual Paulista (UNESP)Hunan Normal UniversitySun, JiaojiaoLiu, YunqiQian, Wei-Liang [UNESP]Chen, SongbaiYue, Ruihong2023-07-29T12:46:21Z2023-07-29T12:46:21Z2023-02-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1088/1674-1137/aca4bcChinese Physics C, v. 47, n. 2, 2023.1674-1137http://hdl.handle.net/11449/24663610.1088/1674-1137/aca4bc2-s2.0-85146189320Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengChinese Physics Cinfo:eu-repo/semantics/openAccess2023-07-29T12:46:21Zoai:repositorio.unesp.br:11449/246636Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T15:45:32.411804Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Black hole shadow in f(R) gravity with nonlinear electrodynamics |
title |
Black hole shadow in f(R) gravity with nonlinear electrodynamics |
spellingShingle |
Black hole shadow in f(R) gravity with nonlinear electrodynamics Sun, Jiaojiao black hole shadow effective metric nonlinear electrodynamics |
title_short |
Black hole shadow in f(R) gravity with nonlinear electrodynamics |
title_full |
Black hole shadow in f(R) gravity with nonlinear electrodynamics |
title_fullStr |
Black hole shadow in f(R) gravity with nonlinear electrodynamics |
title_full_unstemmed |
Black hole shadow in f(R) gravity with nonlinear electrodynamics |
title_sort |
Black hole shadow in f(R) gravity with nonlinear electrodynamics |
author |
Sun, Jiaojiao |
author_facet |
Sun, Jiaojiao Liu, Yunqi Qian, Wei-Liang [UNESP] Chen, Songbai Yue, Ruihong |
author_role |
author |
author2 |
Liu, Yunqi Qian, Wei-Liang [UNESP] Chen, Songbai Yue, Ruihong |
author2_role |
author author author author |
dc.contributor.none.fl_str_mv |
Yangzhou University Universidade de São Paulo (USP) Shanghai Jiao Tong University Universidade Estadual Paulista (UNESP) Hunan Normal University |
dc.contributor.author.fl_str_mv |
Sun, Jiaojiao Liu, Yunqi Qian, Wei-Liang [UNESP] Chen, Songbai Yue, Ruihong |
dc.subject.por.fl_str_mv |
black hole shadow effective metric nonlinear electrodynamics |
topic |
black hole shadow effective metric nonlinear electrodynamics |
description |
By analyzing the propagation of discontinuity in nonlinear electrodynamics, we numerically investigate the related black hole shadows of recently derived rotating black hole solutions in gravity. In this context, the geodesic motion of the relevant perturbations is governed by an effective geometry, which is closely related to the underlying spacetime metric. We derive the effective geometry, and the latter is used to determine the trajectory of the propagation vector of an arbitrary finite discontinuity in the electrodynamic perturbations, namely, the photon. Subsequently, the image of the black hole is evaluated using the ray-tracing technique. Moreover, we discuss the physical relevance of metric parameters, such as the nonlinear coupling, spin, and charge, by studying their impact on the resultant black hole shadows. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-07-29T12:46:21Z 2023-07-29T12:46:21Z 2023-02-01 |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1088/1674-1137/aca4bc Chinese Physics C, v. 47, n. 2, 2023. 1674-1137 http://hdl.handle.net/11449/246636 10.1088/1674-1137/aca4bc 2-s2.0-85146189320 |
url |
http://dx.doi.org/10.1088/1674-1137/aca4bc http://hdl.handle.net/11449/246636 |
identifier_str_mv |
Chinese Physics C, v. 47, n. 2, 2023. 1674-1137 10.1088/1674-1137/aca4bc 2-s2.0-85146189320 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Chinese Physics C |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1808128557297172481 |