Hyperonic equation of state at finite temperature for neutron stars

We review the composition and the equation of state of the hyperonic core of neutron stars at finite temperature within a relativistic mean-field approach. We make use of the new FSU2H∗ model, which is built upon the FSU2H scheme by improving on the Ξ potential according to the recent analysis on th...

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Main Authors: Kochankovski Hristijan, Ramos Angels, Tolos Laura
Format: Article
Language:English
Published: EDP Sciences 2022-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2022/15/epjconf_hyp2022_09005.pdf
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author Kochankovski Hristijan
Ramos Angels
Tolos Laura
author_facet Kochankovski Hristijan
Ramos Angels
Tolos Laura
author_sort Kochankovski Hristijan
collection DOAJ
description We review the composition and the equation of state of the hyperonic core of neutron stars at finite temperature within a relativistic mean-field approach. We make use of the new FSU2H∗ model, which is built upon the FSU2H scheme by improving on the Ξ potential according to the recent analysis on the Ξ atoms, and we extend it to include finite temperature corrections. The calculations are done for a wide range of densities, temperatures and charge fractions, thus exploring the different conditions that can be found in protoneutron stars, binary mergers remnants and supernovae explosions. The inclusion of hyperons has a strong effect on the composition and the equation of state at finite temperature, which consequently would lead to significant changes in the properties and evolution of hot neutron stars.
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spelling doaj.art-05254134a97d4b23937848f3f93d639b2022-12-22T03:42:25ZengEDP SciencesEPJ Web of Conferences2100-014X2022-01-012710900510.1051/epjconf/202227109005epjconf_hyp2022_09005Hyperonic equation of state at finite temperature for neutron starsKochankovski Hristijan0Ramos Angels1Tolos Laura2Departament de Física Quàntica i Astrofísica and Institut de Ciències del Cosmos, Universitat de BarcelonaDepartament de Física Quàntica i Astrofísica and Institut de Ciències del Cosmos, Universitat de BarcelonaInstitute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can MagransWe review the composition and the equation of state of the hyperonic core of neutron stars at finite temperature within a relativistic mean-field approach. We make use of the new FSU2H∗ model, which is built upon the FSU2H scheme by improving on the Ξ potential according to the recent analysis on the Ξ atoms, and we extend it to include finite temperature corrections. The calculations are done for a wide range of densities, temperatures and charge fractions, thus exploring the different conditions that can be found in protoneutron stars, binary mergers remnants and supernovae explosions. The inclusion of hyperons has a strong effect on the composition and the equation of state at finite temperature, which consequently would lead to significant changes in the properties and evolution of hot neutron stars.https://www.epj-conferences.org/articles/epjconf/pdf/2022/15/epjconf_hyp2022_09005.pdf
spellingShingle Kochankovski Hristijan
Ramos Angels
Tolos Laura
Hyperonic equation of state at finite temperature for neutron stars
EPJ Web of Conferences
title Hyperonic equation of state at finite temperature for neutron stars
title_full Hyperonic equation of state at finite temperature for neutron stars
title_fullStr Hyperonic equation of state at finite temperature for neutron stars
title_full_unstemmed Hyperonic equation of state at finite temperature for neutron stars
title_short Hyperonic equation of state at finite temperature for neutron stars
title_sort hyperonic equation of state at finite temperature for neutron stars
url https://www.epj-conferences.org/articles/epjconf/pdf/2022/15/epjconf_hyp2022_09005.pdf
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AT ramosangels hyperonicequationofstateatfinitetemperatureforneutronstars
AT toloslaura hyperonicequationofstateatfinitetemperatureforneutronstars