Isospin Symmetry Breaking Effects on the Mass-Radius Relation of a Neutron Star

Isospin symmetry breaking effects on the mass-radius relation of a cold, non-accreting neutron star are studied on the basis of two Skyrme Energy Density Functionals (EDFs). One functional contains isospin symmetry breaking terms other than those typically included in Skyrme EDFs while its counterpa...

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Main Authors: Giovanni Selva, Xavier Roca-Maza, Gianluca Colò
Format: Article
Language:English
Published: MDPI AG 2021-01-01
Series:Symmetry
Subjects:
Online Access:https://www.mdpi.com/2073-8994/13/1/144
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author Giovanni Selva
Xavier Roca-Maza
Gianluca Colò
author_facet Giovanni Selva
Xavier Roca-Maza
Gianluca Colò
author_sort Giovanni Selva
collection DOAJ
description Isospin symmetry breaking effects on the mass-radius relation of a cold, non-accreting neutron star are studied on the basis of two Skyrme Energy Density Functionals (EDFs). One functional contains isospin symmetry breaking terms other than those typically included in Skyrme EDFs while its counterpart is of standard form. Both functionals are based on the same fitting protocol except for the observables and pseudo-observables sensitive to the isospin symmetry breaking channel. The quality of those functionals is similar in the description of terrestrial observables but choosing either of them has a non-negligible effect on the mass-radius relation and tidal deformability of a neutron star. Further investigations are needed to clarify the effects of isospin symmetry breaking on these and other observables of neutron stars that are, and will become, available.
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spelling doaj.art-8381e8c76dae4385861120676da32f7f2023-12-03T13:28:50ZengMDPI AGSymmetry2073-89942021-01-0113114410.3390/sym13010144Isospin Symmetry Breaking Effects on the Mass-Radius Relation of a Neutron StarGiovanni Selva0Xavier Roca-Maza1Gianluca Colò2Dipartimento di Fisica “Aldo Pontremoli”, Università degli Studi di Milano, Via Giovanni Celoria 16, 20133 Milano, ItalyDipartimento di Fisica “Aldo Pontremoli”, Università degli Studi di Milano, Via Giovanni Celoria 16, 20133 Milano, ItalyDipartimento di Fisica “Aldo Pontremoli”, Università degli Studi di Milano, Via Giovanni Celoria 16, 20133 Milano, ItalyIsospin symmetry breaking effects on the mass-radius relation of a cold, non-accreting neutron star are studied on the basis of two Skyrme Energy Density Functionals (EDFs). One functional contains isospin symmetry breaking terms other than those typically included in Skyrme EDFs while its counterpart is of standard form. Both functionals are based on the same fitting protocol except for the observables and pseudo-observables sensitive to the isospin symmetry breaking channel. The quality of those functionals is similar in the description of terrestrial observables but choosing either of them has a non-negligible effect on the mass-radius relation and tidal deformability of a neutron star. Further investigations are needed to clarify the effects of isospin symmetry breaking on these and other observables of neutron stars that are, and will become, available.https://www.mdpi.com/2073-8994/13/1/144isospin symmetry breakingneutron star mass-radius relationtidal deformability
spellingShingle Giovanni Selva
Xavier Roca-Maza
Gianluca Colò
Isospin Symmetry Breaking Effects on the Mass-Radius Relation of a Neutron Star
Symmetry
isospin symmetry breaking
neutron star mass-radius relation
tidal deformability
title Isospin Symmetry Breaking Effects on the Mass-Radius Relation of a Neutron Star
title_full Isospin Symmetry Breaking Effects on the Mass-Radius Relation of a Neutron Star
title_fullStr Isospin Symmetry Breaking Effects on the Mass-Radius Relation of a Neutron Star
title_full_unstemmed Isospin Symmetry Breaking Effects on the Mass-Radius Relation of a Neutron Star
title_short Isospin Symmetry Breaking Effects on the Mass-Radius Relation of a Neutron Star
title_sort isospin symmetry breaking effects on the mass radius relation of a neutron star
topic isospin symmetry breaking
neutron star mass-radius relation
tidal deformability
url https://www.mdpi.com/2073-8994/13/1/144
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