Can the PREX-2 and CREX results be understood by relativistic mean-field models with the astrophysical constraints?
DC Field | Value | Language |
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dc.contributor.author | Miyatsu, Tsuyoshi | - |
dc.contributor.author | Cheoun, Myung-Ki | - |
dc.contributor.author | Kim, Kyungsik | - |
dc.contributor.author | Saito, Koichi | - |
dc.date.accessioned | 2023-08-02T05:40:04Z | - |
dc.date.available | 2023-08-02T05:40:04Z | - |
dc.date.created | 2023-08-01 | - |
dc.date.issued | 2023-08 | - |
dc.identifier.issn | 0370-2693 | - |
dc.identifier.uri | http://scholarworks.bwise.kr/ssu/handle/2018.sw.ssu/44149 | - |
dc.description.abstract | We construct new effective interactions using the relativistic mean-field models with the isoscalar-and isovector-meson mixing, & sigma;252 and & omega;& mu;& omega;& mu;p & nu;p & nu;. Taking into account the particle flow data in heavy-ion collisions, the observed mass of PSR J0740+6620, and the tidal deformability of a neutron star from the binary merger event, GW170817, we study the ground-state properties of finite, closed-shell nuclei, and try to explain the recent results from the PREX-2 and CREX experiments. It is found that the & sigma;-& delta; mixing is very powerful to understand the terrestrial experiments and astrophysical observations of neutron stars self-consistently. We can predict the large neutron skin thickness of 208Pb, R208 skin = 0.243 fm, using the slope parameter of nuclear symmetry energy, L = 70 MeV, which is consistent with the PREX-2 result. However, to explain the CREX data, it is preferable to adopt the small value of L = 20 MeV. It is very difficult to understand the PREX-2 and CREX results simultaneously within relativistic mean-field models.& COPY; 2023 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons .org /licenses /by /4 .0/). Funded by SCOAP3. | - |
dc.language | 영어 | - |
dc.language.iso | en | - |
dc.publisher | ELSEVIER | - |
dc.relation.isPartOf | PHYSICS LETTERS B | - |
dc.title | Can the PREX-2 and CREX results be understood by relativistic mean-field models with the astrophysical constraints? | - |
dc.type | Article | - |
dc.identifier.doi | 10.1016/j.physletb.2023.138013 | - |
dc.type.rims | ART | - |
dc.identifier.bibliographicCitation | PHYSICS LETTERS B, v.843 | - |
dc.description.journalClass | 1 | - |
dc.identifier.wosid | 001025621700001 | - |
dc.identifier.scopusid | 2-s2.0-85162027590 | - |
dc.citation.title | PHYSICS LETTERS B | - |
dc.citation.volume | 843 | - |
dc.contributor.affiliatedAuthor | Cheoun, Myung-Ki | - |
dc.identifier.url | https://www.sciencedirect.com/science/article/pii/S0370269323003477?via%3Dihub | - |
dc.type.docType | Article | - |
dc.description.isOpenAccess | Y | - |
dc.subject.keywordAuthor | Relativistic mean-field models | - |
dc.subject.keywordAuthor | PREX-2 and CREX experiments | - |
dc.subject.keywordAuthor | Isospin-asymmetric nuclear matter | - |
dc.subject.keywordAuthor | Neutron stars | - |
dc.subject.keywordPlus | MESON COUPLING MODEL | - |
dc.subject.keywordPlus | SYMMETRY ENERGY | - |
dc.subject.keywordPlus | NUCLEAR | - |
dc.subject.keywordPlus | STATE | - |
dc.subject.keywordPlus | TERM | - |
dc.subject.keywordPlus | EQUATION | - |
dc.subject.keywordPlus | MATTER | - |
dc.relation.journalResearchArea | Astronomy & Astrophysics | - |
dc.relation.journalResearchArea | Physics | - |
dc.relation.journalWebOfScienceCategory | Astronomy & Astrophysics | - |
dc.relation.journalWebOfScienceCategory | Physics, Nuclear | - |
dc.relation.journalWebOfScienceCategory | Physics, Particles & Fields | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
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