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spelling I65-R171-20.500.12049-28302023-09-13T15:35:32Z application/pdf info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/4.0/ 2016-12-22 Fil: Teppa Pannia, Florencia A. Comisión de Investigaciones Científicas; Argentina Fil: Teppa Pannia, Florencia A. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Teppa Pannia, Florencia A. Instituto Argentino de Radioastronomía; Argentina Fil: García, Federico. Comisión de Investigaciones Científicas; Argentina Fil: García, Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: García, Federico. Instituto Argentino de Radioastronomía; Argentina Fil: Perez Bergliaffa, Santiago E. Universidade Do Estado Do Rio de Janeiro; Brasil Fil: Orellana, Mariana D. Universidad Nacional de Rio Negro. Sede Andina; Argentina Fil: Romero, Gustavo E. Comisión de Investigaciones Científicas; Argentina Fil: Romero, Gustavo E. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Romero, Gustavo E. Instituto Argentino de Radioastronomia; Argentina Structure of compact stars in R-squared Palatini gravity Teppa Pannia, Florencia A. García, Federico Perez Bergliaffa, Santiago E. Orellana, Mariana Dominga Romero, Gustavo E. Ciencias Físicas Modified Gravity Palatini Formalism Neutron Stars Equation of State Ciencias Físicas true We analyse configurations of neutron stars in the so-called R-squared gravity in the Palatini formalism. Using a realistic equation of state we show that the mass-radius configurations are lighter than their counterparts in General Relativity. We also obtain the internal profiles, which run in strong correlation with the derivatives of the equation of state, leading to regions where the mass parameter decreases with the radial coordinate in a counter-intuitive way. In order to analyse such correlation, we introduce a parametrisation of the equation of state given by multiple polytropes, which allows us to explicitly control its derivatives. We show that, even in a limiting case where hard phase transitions in matter are allowed, the internal profile of the mass parameter still presents strange features and the calculated M −R configurations also yield neutron stars lighter than those obtained in General Relativity. Teppa Pannia, Florencia A., García, Federico., Perez Bergliaffa, Santiago E., Orellana, Mariana D. & Romero, Gustavo E. (2016). Structure of compact stars in R-squared Palatini gravity. Springer/Plenum Publishers; General Relativity And Gravitation; 49; 2; 1-14 0001-7701 http://link.springer.com/article/10.1007/s10714-016-2182-7 http://dx.doi.org/10.1007/s10714-016-2182-7 http://hdl.handle.net/11336/63359 https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2830 eng General Relativity And Gravitation
institution Universidad Nacional de Río Negro
institution_str I-65
repository_str R-171
collection Repositorio Institucional Digital de la Universidad Nacional de Río Negro (UNRN)
language Inglés
orig_language_str_mv eng
topic Ciencias Físicas
Modified Gravity
Palatini Formalism
Neutron Stars
Equation of State
Ciencias Físicas
spellingShingle Ciencias Físicas
Modified Gravity
Palatini Formalism
Neutron Stars
Equation of State
Ciencias Físicas
Teppa Pannia, Florencia A.
García, Federico
Perez Bergliaffa, Santiago E.
Orellana, Mariana Dominga
Romero, Gustavo E.
Structure of compact stars in R-squared Palatini gravity
topic_facet Ciencias Físicas
Modified Gravity
Palatini Formalism
Neutron Stars
Equation of State
Ciencias Físicas
description Fil: Teppa Pannia, Florencia A. Comisión de Investigaciones Científicas; Argentina
author Teppa Pannia, Florencia A.
García, Federico
Perez Bergliaffa, Santiago E.
Orellana, Mariana Dominga
Romero, Gustavo E.
author_facet Teppa Pannia, Florencia A.
García, Federico
Perez Bergliaffa, Santiago E.
Orellana, Mariana Dominga
Romero, Gustavo E.
author_sort Teppa Pannia, Florencia A.
title Structure of compact stars in R-squared Palatini gravity
title_short Structure of compact stars in R-squared Palatini gravity
title_full Structure of compact stars in R-squared Palatini gravity
title_fullStr Structure of compact stars in R-squared Palatini gravity
title_full_unstemmed Structure of compact stars in R-squared Palatini gravity
title_sort structure of compact stars in r-squared palatini gravity
publishDate 2016
url http://link.springer.com/article/10.1007/s10714-016-2182-7
http://dx.doi.org/10.1007/s10714-016-2182-7
http://hdl.handle.net/11336/63359
https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2830
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