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spelling I65-R171-20.500.12049-28312023-09-13T15:35:41Z application/pdf info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/4.0/ 2013-06-22 Fil: Orellana, Mariana D. Universidad Nacional de Río Negro; Argentina Fil: Orellana, Mariana D. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Orellana, Mariana D. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Fil: Orellana, Mariana D. Instituto Argentino de Radioastronomia; Argentina Fil: García, Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina Fil: García, Federico. Instituto Argentino de Radioastronomia; Argentina. Fil: García, Federico. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Teppa Pannia, Florencia A. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Romero, Gustavo E. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina Fil: Romero, Gustavo E. Instituto Argentino de Radioastronomia; Argentina. Fil: Romero, Gustavo E. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Structure of neutron stars in R-squared gravity Orellana, Mariana Dominga García, Federico Teppa Pannia, Florencia A. Romero, Gustavo E. Ciencias Físicas Modified Gravity Neutron Stars Generalised Gravity Equation Ciencias Físicas true The 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. Orellana, 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 0001-7701 http://link.springer.com/article/10.1007%2Fs10714-013-1501-5 http://arxiv.org/abs/1301.5189 https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2831 http://dx.doi.org/10.1007/s10714-013-1501-5 eng 45 General Relativity And Gravitation Springer
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
Neutron Stars
Generalised Gravity Equation
Ciencias Físicas
spellingShingle Ciencias Físicas
Modified Gravity
Neutron Stars
Generalised Gravity Equation
Ciencias Físicas
Orellana, Mariana Dominga
García, Federico
Teppa Pannia, Florencia A.
Romero, Gustavo E.
Structure of neutron stars in R-squared gravity
topic_facet Ciencias Físicas
Modified Gravity
Neutron Stars
Generalised Gravity Equation
Ciencias Físicas
description Fil: Orellana, Mariana D. Universidad Nacional de Río Negro; Argentina
author Orellana, Mariana Dominga
García, Federico
Teppa Pannia, Florencia A.
Romero, Gustavo E.
author_facet Orellana, Mariana Dominga
García, Federico
Teppa Pannia, Florencia A.
Romero, Gustavo E.
author_sort Orellana, Mariana Dominga
title Structure of neutron stars in R-squared gravity
title_short Structure of neutron stars in R-squared gravity
title_full Structure of neutron stars in R-squared gravity
title_fullStr Structure of neutron stars in R-squared gravity
title_full_unstemmed Structure of neutron stars in R-squared gravity
title_sort structure of neutron stars in r-squared gravity
publisher Springer
publishDate 2013
url http://link.springer.com/article/10.1007%2Fs10714-013-1501-5
http://arxiv.org/abs/1301.5189
https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2831
http://dx.doi.org/10.1007/s10714-013-1501-5
work_keys_str_mv AT orellanamarianadominga structureofneutronstarsinrsquaredgravity
AT garciafederico structureofneutronstarsinrsquaredgravity
AT teppapanniaflorenciaa structureofneutronstarsinrsquaredgravity
AT romerogustavoe structureofneutronstarsinrsquaredgravity
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