Constraints on Nuclear Saturation Properties from Terrestrial Experiments and Astrophysical Observations of Neutron Stars
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Choi, Soonchul | - |
dc.contributor.author | Miyatsu, Tsuyoshi | - |
dc.contributor.author | Cheoun, Myung-Ki | - |
dc.contributor.author | Saito, Koichi | - |
dc.date.available | 2021-03-23T03:40:13Z | - |
dc.date.created | 2021-03-23 | - |
dc.date.issued | 2021-03 | - |
dc.identifier.issn | 0004-637X | - |
dc.identifier.uri | http://scholarworks.bwise.kr/ssu/handle/2018.sw.ssu/40720 | - |
dc.description.abstract | Taking into account the terrestrial experiments and the recent astrophysical observations of neutron stars and gravitational-wave signals, we impose restrictions on the equation of state (EoS) for isospin-asymmetric nuclear matter. Using the relativistic mean-field model with SU(3) flavor symmetry, we investigate the impacts of effective nucleon mass, nuclear incompressibility, and slope parameter of nuclear symmetry energy on the nuclear and neutron star properties. It is found that the astrophysical information of massive neutron stars and tidal deformabilities, as well as the nuclear experimental data, plays an important role to restrict the EoS for neutron stars. In particular, the softness of the nuclear EoS due to the existence of hyperons in the core gives stringent constraints on those physical quantities. Furthermore, it is possible to put limits on the curvature parameter of nuclear symmetry energy by means of nuclear and astrophysical calculations. | - |
dc.language | 영어 | - |
dc.language.iso | en | - |
dc.publisher | IOP PUBLISHING LTD | - |
dc.relation.isPartOf | ASTROPHYSICAL JOURNAL | - |
dc.title | Constraints on Nuclear Saturation Properties from Terrestrial Experiments and Astrophysical Observations of Neutron Stars | - |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/abe3fe | - |
dc.type.rims | ART | - |
dc.identifier.bibliographicCitation | ASTROPHYSICAL JOURNAL, v.909, no.2 | - |
dc.description.journalClass | 1 | - |
dc.identifier.wosid | 000629138600001 | - |
dc.identifier.scopusid | 2-s2.0-85103233886 | - |
dc.citation.number | 2 | - |
dc.citation.title | ASTROPHYSICAL JOURNAL | - |
dc.citation.volume | 909 | - |
dc.contributor.affiliatedAuthor | Cheoun, Myung-Ki | - |
dc.type.docType | Article | - |
dc.description.isOpenAccess | N | - |
dc.subject.keywordAuthor | Neutron stars | - |
dc.subject.keywordAuthor | Nuclear astrophysics | - |
dc.subject.keywordAuthor | Nuclear physics | - |
dc.subject.keywordPlus | SCATTERING | - |
dc.subject.keywordPlus | PHYSICS | - |
dc.subject.keywordPlus | ENERGY | - |
dc.subject.keywordPlus | MATTER | - |
dc.relation.journalResearchArea | Astronomy & Astrophysics | - |
dc.relation.journalWebOfScienceCategory | Astronomy & Astrophysics | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
Items in ScholarWorks are protected by copyright, with all rights reserved, unless otherwise indicated.
Soongsil University Library 369 Sangdo-Ro, Dongjak-Gu, Seoul, Korea (06978)02-820-0733
COPYRIGHT ⓒ SOONGSIL UNIVERSITY, ALL RIGHTS RESERVED.
Certain data included herein are derived from the © Web of Science of Clarivate Analytics. All rights reserved.
You may not copy or re-distribute this material in whole or in part without the prior written consent of Clarivate Analytics.