An analysis of a regular black hole interior
In this work we address the issue of the thermodynamic behavior of a non-singular spherically-symmetric black hole model introduced by Mbonye and Kanzanas (2005). This spacetime is described by Schwarschild’s solution at large radius and by a de Sitterlike solution at small radius. The interior of t...
| Autores: | , , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2011 |
| País: | Argentina |
| Institución: | Consejo Nacional de Investigaciones Científicas y Técnicas |
| Repositorio: | CONICET Digital (CONICET) |
| Idioma: | inglés |
| OAI Identifier: | oai:ri.conicet.gov.ar:11336/5909 |
| Acceso en línea: | http://hdl.handle.net/11336/5909 |
| Access Level: | acceso abierto |
| Palabra clave: | Black Holes Gravitation Singularity https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| id |
AR_7d5d813cfc10b7ba2e09c4e8f2975dcd |
|---|---|
| oai_identifier_str |
oai:ri.conicet.gov.ar:11336/5909 |
| network_acronym_str |
AR |
| network_name_str |
Argentina |
| repository_id_str |
|
| spelling |
An analysis of a regular black hole interiorPérez, DanielaRomero, Gustavo EstebanCorrea, Camila A.Perez Bergliaffa, Santiago EstebanBlack HolesGravitationSingularityhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In this work we address the issue of the thermodynamic behavior of a non-singular spherically-symmetric black hole model introduced by Mbonye and Kanzanas (2005). This spacetime is described by Schwarschild’s solution at large radius and by a de Sitterlike solution at small radius. The interior of the black hole consists of matter fields with sound speed bounded by the speed of light. The matter transits smoothly between normal matter and a core of an exotic fluid with an equation of state that approaches p = −ρ when r → 0. We derive the general equations of the thermodynamic quantities for an arbitrary matter density profile, and adjust the results to the specific regular black hole. We also calculate the Weyl and Kretschmann scalars and analyse the behaviour of the gravitational field in connection with the thermodynamics of the matter fields. Finally, we study whether the regular behaviour at the center affects the thermodynamics of the black hole, and we discuss a possible physical interpretation of the state of regular black hole interiors.Fil: Pérez, Daniela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); ArgentinaFil: Romero, Gustavo Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); ArgentinaFil: Correa, Camila A.. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Perez Bergliaffa, Santiago Esteban. Universidade do Estado do Rio de Janeiro. Departamento de Física Teórica, Instituto de Física; BrasilWorld Scientific2011-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/5909Pérez, Daniela; Romero, Gustavo Esteban; Correa, Camila A.; Perez Bergliaffa, Santiago Esteban; An analysis of a regular black hole interior; World Scientific; International Journal of Modern Physics: Conference Series; 3; 1-2011; 396-4072010-1945enginfo:eu-repo/semantics/altIdentifier/doi/10.1142/S2010194511001498info:eu-repo/semantics/altIdentifier/url/http://www.worldscientific.com/doi/abs/10.1142/S2010194511001498info:eu-repo/semantics/openAccessAtribución-NoComercial-CompartirIgual 2.5 Argentina (CC BY-NC-SA 2.5 AR)https://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2024-05-08T13:56:04Zoai:ri.conicet.gov.ar:11336/5909instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982024-05-08 13:56:04.577CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
An analysis of a regular black hole interior |
| title |
An analysis of a regular black hole interior |
| spellingShingle |
An analysis of a regular black hole interior Pérez, Daniela Black Holes Gravitation Singularity https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| title_short |
An analysis of a regular black hole interior |
| title_full |
An analysis of a regular black hole interior |
| title_fullStr |
An analysis of a regular black hole interior |
| title_full_unstemmed |
An analysis of a regular black hole interior |
| title_sort |
An analysis of a regular black hole interior |
| dc.creator.none.fl_str_mv |
Pérez, Daniela Romero, Gustavo Esteban Correa, Camila A. Perez Bergliaffa, Santiago Esteban |
| author |
Pérez, Daniela |
| author_facet |
Pérez, Daniela Romero, Gustavo Esteban Correa, Camila A. Perez Bergliaffa, Santiago Esteban |
| author_role |
author |
| author2 |
Romero, Gustavo Esteban Correa, Camila A. Perez Bergliaffa, Santiago Esteban |
| author2_role |
author author author |
| dc.subject.none.fl_str_mv |
Black Holes Gravitation Singularity https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| topic |
Black Holes Gravitation Singularity https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| description |
In this work we address the issue of the thermodynamic behavior of a non-singular spherically-symmetric black hole model introduced by Mbonye and Kanzanas (2005). This spacetime is described by Schwarschild’s solution at large radius and by a de Sitterlike solution at small radius. The interior of the black hole consists of matter fields with sound speed bounded by the speed of light. The matter transits smoothly between normal matter and a core of an exotic fluid with an equation of state that approaches p = −ρ when r → 0. We derive the general equations of the thermodynamic quantities for an arbitrary matter density profile, and adjust the results to the specific regular black hole. We also calculate the Weyl and Kretschmann scalars and analyse the behaviour of the gravitational field in connection with the thermodynamics of the matter fields. Finally, we study whether the regular behaviour at the center affects the thermodynamics of the black hole, and we discuss a possible physical interpretation of the state of regular black hole interiors. |
| publishDate |
2011 |
| dc.date.none.fl_str_mv |
2011-01 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/5909 Pérez, Daniela; Romero, Gustavo Esteban; Correa, Camila A.; Perez Bergliaffa, Santiago Esteban; An analysis of a regular black hole interior; World Scientific; International Journal of Modern Physics: Conference Series; 3; 1-2011; 396-407 2010-1945 |
| url |
http://hdl.handle.net/11336/5909 |
| identifier_str_mv |
Pérez, Daniela; Romero, Gustavo Esteban; Correa, Camila A.; Perez Bergliaffa, Santiago Esteban; An analysis of a regular black hole interior; World Scientific; International Journal of Modern Physics: Conference Series; 3; 1-2011; 396-407 2010-1945 |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
| dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1142/S2010194511001498 info:eu-repo/semantics/altIdentifier/url/http://www.worldscientific.com/doi/abs/10.1142/S2010194511001498 |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess Atribución-NoComercial-CompartirIgual 2.5 Argentina (CC BY-NC-SA 2.5 AR) https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
| eu_rights_str_mv |
openAccess |
| rights_invalid_str_mv |
Atribución-NoComercial-CompartirIgual 2.5 Argentina (CC BY-NC-SA 2.5 AR) https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
| dc.format.none.fl_str_mv |
application/pdf application/pdf |
| dc.publisher.none.fl_str_mv |
World Scientific |
| publisher.none.fl_str_mv |
World Scientific |
| dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
| instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
| reponame_str |
CONICET Digital (CONICET) |
| collection |
CONICET Digital (CONICET) |
| repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
| repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
| _version_ |
1799195553179893760 |
| score |
15,812455 |