Traversable thin-shell wormhole in the 4D Einstein–Gauss–Bonnet theory
Autor(a) principal: | |
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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/10.1016/j.cjph.2023.04.016 http://hdl.handle.net/11449/247391 |
Resumo: | This work investigates the spherically symmetric thin-shell wormhole solutions in four-dimensional Einstein–Gauss–Bonnet theory and explores their stabilities under radial, linear perturbations. These solutions are typically traversable and characterized by a thin-shell throat in accordance with Israel's junction conditions. In asymptotically flat and AdS spacetimes with a negative Gauss–Bonnet coupling constant, stable neutral wormholes are encountered when the magnitude of the coupling constant becomes significant. The throats of such wormholes are sustained by ordinary matter and possess finite radii. In asymptotically dS spacetimes, no stable neutral wormhole featuring ordinary matter is observed. On the other hand, for positive Gauss–Bonnet coupling constant, stable thin-shell wormhole solutions can be established when the throats are exclusively supported by exotic matter. Moreover, stable charged wormholes comprised of ordinary matter are found universally in the asymptotically flat, AdS, and dS spacetimes. Unlike their neutral counterparts, the throat radii of such charged wormholes can be arbitrarily small. However, as the charge becomes more significant, such solutions only remain stable when supported by exotic matter. |
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Traversable thin-shell wormhole in the 4D Einstein–Gauss–Bonnet theory4D Einstein–Gauss–Bonnet theoryThin-shell wormholeThis work investigates the spherically symmetric thin-shell wormhole solutions in four-dimensional Einstein–Gauss–Bonnet theory and explores their stabilities under radial, linear perturbations. These solutions are typically traversable and characterized by a thin-shell throat in accordance with Israel's junction conditions. In asymptotically flat and AdS spacetimes with a negative Gauss–Bonnet coupling constant, stable neutral wormholes are encountered when the magnitude of the coupling constant becomes significant. The throats of such wormholes are sustained by ordinary matter and possess finite radii. In asymptotically dS spacetimes, no stable neutral wormhole featuring ordinary matter is observed. On the other hand, for positive Gauss–Bonnet coupling constant, stable thin-shell wormhole solutions can be established when the throats are exclusively supported by exotic matter. Moreover, stable charged wormholes comprised of ordinary matter are found universally in the asymptotically flat, AdS, and dS spacetimes. Unlike their neutral counterparts, the throat radii of such charged wormholes can be arbitrarily small. However, as the charge becomes more significant, such solutions only remain stable when supported by exotic matter.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Fundação de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ)Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)National Natural Science Foundation of ChinaBasic and Applied Basic Research Foundation of Guangdong ProvinceDepartment of Physics and Siyuan Laboratory Jinan UniversityCollege of Science Beijing Information Science and Technology UniversityEscola de Engenharia de Lorena Universidade de São PauloFaculdade de Engenharia de Guaratinguetá Universidade Estadual PaulistaCenter for Gravitation and Cosmology College of Physical Science and Technology Yangzhou UniversityFaculdade de Engenharia de Guaratinguetá Universidade Estadual PaulistaNational Natural Science Foundation of China: 11805083National Natural Science Foundation of China: 11847055National Natural Science Foundation of China: 11905083National Natural Science Foundation of China: 11947067National Natural Science Foundation of China: 12005077Basic and Applied Basic Research Foundation of Guangdong Province: 2021A1515012374Jinan UniversityBeijing Information Science and Technology UniversityUniversidade de São Paulo (USP)Universidade Estadual Paulista (UNESP)Yangzhou UniversityZhang, Cheng-YongNiu, ChaoQian, Wei-Liang [UNESP]Wang, XiaobaoLiu, Peng2023-07-29T13:14:48Z2023-07-29T13:14:48Z2023-06-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article527-538http://dx.doi.org/10.1016/j.cjph.2023.04.016Chinese Journal of Physics, v. 83, p. 527-538.0577-9073http://hdl.handle.net/11449/24739110.1016/j.cjph.2023.04.0162-s2.0-85159449593Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengChinese Journal of Physicsinfo:eu-repo/semantics/openAccess2023-07-29T13:14:48Zoai:repositorio.unesp.br:11449/247391Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T15:01:38.933724Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Traversable thin-shell wormhole in the 4D Einstein–Gauss–Bonnet theory |
title |
Traversable thin-shell wormhole in the 4D Einstein–Gauss–Bonnet theory |
spellingShingle |
Traversable thin-shell wormhole in the 4D Einstein–Gauss–Bonnet theory Zhang, Cheng-Yong 4D Einstein–Gauss–Bonnet theory Thin-shell wormhole |
title_short |
Traversable thin-shell wormhole in the 4D Einstein–Gauss–Bonnet theory |
title_full |
Traversable thin-shell wormhole in the 4D Einstein–Gauss–Bonnet theory |
title_fullStr |
Traversable thin-shell wormhole in the 4D Einstein–Gauss–Bonnet theory |
title_full_unstemmed |
Traversable thin-shell wormhole in the 4D Einstein–Gauss–Bonnet theory |
title_sort |
Traversable thin-shell wormhole in the 4D Einstein–Gauss–Bonnet theory |
author |
Zhang, Cheng-Yong |
author_facet |
Zhang, Cheng-Yong Niu, Chao Qian, Wei-Liang [UNESP] Wang, Xiaobao Liu, Peng |
author_role |
author |
author2 |
Niu, Chao Qian, Wei-Liang [UNESP] Wang, Xiaobao Liu, Peng |
author2_role |
author author author author |
dc.contributor.none.fl_str_mv |
Jinan University Beijing Information Science and Technology University Universidade de São Paulo (USP) Universidade Estadual Paulista (UNESP) Yangzhou University |
dc.contributor.author.fl_str_mv |
Zhang, Cheng-Yong Niu, Chao Qian, Wei-Liang [UNESP] Wang, Xiaobao Liu, Peng |
dc.subject.por.fl_str_mv |
4D Einstein–Gauss–Bonnet theory Thin-shell wormhole |
topic |
4D Einstein–Gauss–Bonnet theory Thin-shell wormhole |
description |
This work investigates the spherically symmetric thin-shell wormhole solutions in four-dimensional Einstein–Gauss–Bonnet theory and explores their stabilities under radial, linear perturbations. These solutions are typically traversable and characterized by a thin-shell throat in accordance with Israel's junction conditions. In asymptotically flat and AdS spacetimes with a negative Gauss–Bonnet coupling constant, stable neutral wormholes are encountered when the magnitude of the coupling constant becomes significant. The throats of such wormholes are sustained by ordinary matter and possess finite radii. In asymptotically dS spacetimes, no stable neutral wormhole featuring ordinary matter is observed. On the other hand, for positive Gauss–Bonnet coupling constant, stable thin-shell wormhole solutions can be established when the throats are exclusively supported by exotic matter. Moreover, stable charged wormholes comprised of ordinary matter are found universally in the asymptotically flat, AdS, and dS spacetimes. Unlike their neutral counterparts, the throat radii of such charged wormholes can be arbitrarily small. However, as the charge becomes more significant, such solutions only remain stable when supported by exotic matter. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-07-29T13:14:48Z 2023-07-29T13:14:48Z 2023-06-01 |
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/10.1016/j.cjph.2023.04.016 Chinese Journal of Physics, v. 83, p. 527-538. 0577-9073 http://hdl.handle.net/11449/247391 10.1016/j.cjph.2023.04.016 2-s2.0-85159449593 |
url |
http://dx.doi.org/10.1016/j.cjph.2023.04.016 http://hdl.handle.net/11449/247391 |
identifier_str_mv |
Chinese Journal of Physics, v. 83, p. 527-538. 0577-9073 10.1016/j.cjph.2023.04.016 2-s2.0-85159449593 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Chinese Journal of Physics |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
527-538 |
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_ |
1808128448678330368 |