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dc.provenanceUniversidad Nacional de Río Negro-
dc.creatorOrellana, Mariana D.-
dc.creatorGarcía, Federico-
dc.creatorTeppa Pannia, Florencia A.-
dc.creatorRomero, Gustavo E.-
dc.date2013-06-22-
dc.date.accessioned2020-02-11T14:09:29Z-
dc.date.available2020-02-11T14:09:29Z-
dc.date.issued2013-06-22-
dc.identifierOrellana, Mariana D., García, Federico., Teppa Pannia, Florencia A. & Romero, Gustavo E. (2013). Structure of neutron stars in R-squared gravity. Springer; General Relativity And Gravitation; 45; 4; 771-783-
dc.identifier0001-7701-
dc.identifierhttp://link.springer.com/article/10.1007%2Fs10714-013-1501-5-
dc.identifierhttp://arxiv.org/abs/1301.5189-
dc.identifierhttps://rid.unrn.edu.ar/jspui/handle/20.500.12049/2831-
dc.identifierhttp://dx.doi.org/10.1007/s10714-013-1501-5-
dc.identifier.urihttp://rodna.bn.gov.ar/jspui/handle/bnmm/575891-
dc.descriptionFil: Orellana, Mariana D. Universidad Nacional de Río Negro; Argentina-
dc.descriptionFil: Orellana, Mariana D. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina-
dc.descriptionFil: Orellana, Mariana D. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina.-
dc.descriptionFil: Orellana, Mariana D. Instituto Argentino de Radioastronomia; Argentina-
dc.descriptionFil: García, Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina-
dc.descriptionFil: García, Federico. Instituto Argentino de Radioastronomia; Argentina.-
dc.descriptionFil: García, Federico. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina-
dc.descriptionFil: Teppa Pannia, Florencia A. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina-
dc.descriptionFil: Romero, Gustavo E. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina-
dc.descriptionFil: Romero, Gustavo E. Instituto Argentino de Radioastronomia; Argentina.-
dc.descriptionFil: Romero, Gustavo E. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina-
dc.descriptionThe effects implied for the structure of compact objects by the modification of General Relativity produced by the generalization of the Lagrangian density to the form R plus alpha R-squared, where R is the Ricci curvature scalar, have been recently explored. It seems likely that this squared-gravity may allow heavier Neutron Stars (NSs) than GR. In addition, these objects can be useful to constrain free parameters of modified-gravity theories. The differences between alternative gravity theories is enhanced in the strong gravitational regime. In this regime, because of the complexity of the field equations, perturbative methods become a good choice to treat the problem. Following previous works in the field, we performed a numerical integration of the structure equations that describe NSs in f(R)-gravity, recovering their mass-radius relations, but focusing on particular features that arise from this approach in the profiles of the NS interior.We show that these profiles run in correlation with the second-order derivative of the analytic approximation to the Equation of State (EoS), which leads to regions where the enclosed mass decreases with the radius in a counter-intuitive way. We reproduce all computations with a simple polytropic EoS to separate zeroth-order modified gravity effects.-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherSpringer-
dc.relation45-
dc.relationGeneral Relativity And Gravitation-
dc.rightsinfo:eu-repo/semantics/openAccess-
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/4.0/-
dc.sourcereponame:RID-UNRN (UNRN)-
dc.sourceinstname:Universidad Nacional de Río Negro-
dc.sourceinstacron:UNRN-
dc.source.urihttp://dx.doi.org/10.1007/s10714-013-1501-5-
dc.subjectModified Gravity-
dc.subjectNeutron Stars-
dc.subjectGeneralised Gravity Equation-
dc.subject.::Ciencias Exactas y Naturales::Ciencias Físicas-
dc.titleStructure of neutron stars in R-squared gravity-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/acceptedVersion-
dc.typeinfo:ar-repo/semantics/articulo-
dc.about-
Aparece en las colecciones: Universidad Nacional de Río Negro

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