Structure of compact stars in Palatini f (R) gravity
- Autores
- García, Federico; Teppa Pannia, Florencia Anabella; Pérez Bergliaffa, Santiago Esteban; Orellana, Mariana Dominga; Romero, Gustavo Esteban
- Año de publicación
- 2014
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- The study of the structure of compact objects in modified theories of gravity can be useful to constrain f (R)-theories in the strong gravitational regime. In particular, the structure of compact stars in the theory with Langrangian density f (R) = R + αR2 have been recently explored using the metric formalism. In this work we analyze configurations of neutron stars in squared-gravity using the Palatini formalism, in which the field equations are of second order, and the modified Tolman-Oppenheimer-Volkoff equations for a sphericallysymmetric and static metric can be derived without approximation, as in General Relativity. The numerical integration of the structure equations allows us to study the mass-radius configurations and the characteristics of internal profiles. We compare our results with those obtained using General Relativity.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
neutron stars
Palatini formalism
modified gravity - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/165283
Ver los metadatos del registro completo
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Structure of compact stars in Palatini f (R) gravityGarcía, FedericoTeppa Pannia, Florencia AnabellaPérez Bergliaffa, Santiago EstebanOrellana, Mariana DomingaRomero, Gustavo EstebanCiencias Astronómicasneutron starsPalatini formalismmodified gravityThe study of the structure of compact objects in modified theories of gravity can be useful to constrain f (R)-theories in the strong gravitational regime. In particular, the structure of compact stars in the theory with Langrangian density f (R) = R + αR2 have been recently explored using the metric formalism. In this work we analyze configurations of neutron stars in squared-gravity using the Palatini formalism, in which the field equations are of second order, and the modified Tolman-Oppenheimer-Volkoff equations for a sphericallysymmetric and static metric can be derived without approximation, as in General Relativity. The numerical integration of the structure equations allows us to study the mass-radius configurations and the characteristics of internal profiles. We compare our results with those obtained using General Relativity.Facultad de Ciencias Astronómicas y Geofísicas2014-04info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf207-210http://sedici.unlp.edu.ar/handle/10915/165283enginfo:eu-repo/semantics/altIdentifier/isbn/978-987-24948-2-7info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-03T11:15:44Zoai:sedici.unlp.edu.ar:10915/165283Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 11:15:45.173SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Structure of compact stars in Palatini f (R) gravity |
title |
Structure of compact stars in Palatini f (R) gravity |
spellingShingle |
Structure of compact stars in Palatini f (R) gravity García, Federico Ciencias Astronómicas neutron stars Palatini formalism modified gravity |
title_short |
Structure of compact stars in Palatini f (R) gravity |
title_full |
Structure of compact stars in Palatini f (R) gravity |
title_fullStr |
Structure of compact stars in Palatini f (R) gravity |
title_full_unstemmed |
Structure of compact stars in Palatini f (R) gravity |
title_sort |
Structure of compact stars in Palatini f (R) gravity |
dc.creator.none.fl_str_mv |
García, Federico Teppa Pannia, Florencia Anabella Pérez Bergliaffa, Santiago Esteban Orellana, Mariana Dominga Romero, Gustavo Esteban |
author |
García, Federico |
author_facet |
García, Federico Teppa Pannia, Florencia Anabella Pérez Bergliaffa, Santiago Esteban Orellana, Mariana Dominga Romero, Gustavo Esteban |
author_role |
author |
author2 |
Teppa Pannia, Florencia Anabella Pérez Bergliaffa, Santiago Esteban Orellana, Mariana Dominga Romero, Gustavo Esteban |
author2_role |
author author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas neutron stars Palatini formalism modified gravity |
topic |
Ciencias Astronómicas neutron stars Palatini formalism modified gravity |
dc.description.none.fl_txt_mv |
The study of the structure of compact objects in modified theories of gravity can be useful to constrain f (R)-theories in the strong gravitational regime. In particular, the structure of compact stars in the theory with Langrangian density f (R) = R + αR2 have been recently explored using the metric formalism. In this work we analyze configurations of neutron stars in squared-gravity using the Palatini formalism, in which the field equations are of second order, and the modified Tolman-Oppenheimer-Volkoff equations for a sphericallysymmetric and static metric can be derived without approximation, as in General Relativity. The numerical integration of the structure equations allows us to study the mass-radius configurations and the characteristics of internal profiles. We compare our results with those obtained using General Relativity. Facultad de Ciencias Astronómicas y Geofísicas |
description |
The study of the structure of compact objects in modified theories of gravity can be useful to constrain f (R)-theories in the strong gravitational regime. In particular, the structure of compact stars in the theory with Langrangian density f (R) = R + αR2 have been recently explored using the metric formalism. In this work we analyze configurations of neutron stars in squared-gravity using the Palatini formalism, in which the field equations are of second order, and the modified Tolman-Oppenheimer-Volkoff equations for a sphericallysymmetric and static metric can be derived without approximation, as in General Relativity. The numerical integration of the structure equations allows us to study the mass-radius configurations and the characteristics of internal profiles. We compare our results with those obtained using General Relativity. |
publishDate |
2014 |
dc.date.none.fl_str_mv |
2014-04 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/conferenceObject info:eu-repo/semantics/publishedVersion Objeto de conferencia http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
format |
conferenceObject |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/165283 |
url |
http://sedici.unlp.edu.ar/handle/10915/165283 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/isbn/978-987-24948-2-7 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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application/pdf 207-210 |
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