Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Shishao Bao"'
Publikováno v:
Physical Review C. 104
The secondary component of GW190814 with a mass of 2.50--2.67 ${M}_{\ensuremath{\bigodot}}$ may be the lightest black hole or the heaviest neutron star ever observed in a binary compact object system. To explore the possible equation of state (EOS),
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b6cc13401f95aba10335e603018b52f1
https://doi.org/10.1103/physrevc.104.015802
https://doi.org/10.1103/physrevc.104.015802
We study the impact of strong magnetic fields on the pasta phases that are expected to exist in the inner crust of neutron stars. We employ the relativistic mean field model to describe the nucleon interaction and use the self-consistent Thomas-Fermi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d3163ba789c5780abe3a760a1f9c567e
http://arxiv.org/abs/2101.04868
http://arxiv.org/abs/2101.04868
Publikováno v:
Progress of Theoretical and Experimental Physics. 2020
The radii and tidal deformabilities of neutron stars are investigated in the framework of the relativistic mean-field (RMF) model with different density-dependent behaviors of symmetry energy. To study the effects of symmetry energy on the properties
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::efe1472d7cdb4380944ab3ceb11fc8c0
https://doi.org/10.1093/ptep/ptaa016
https://doi.org/10.1093/ptep/ptaa016
Publikováno v:
Chinese Science Bulletin. 63:828-835
It is generally believed that a neutron star mainly consists of four parts,that is to say, outer crust, inner crust, outer core, and inner core.From neutron drip density to crust-core transition density,the inner crust of neutron star is a nonuniform
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5f85fb871257d90c81ffc514bd09cd93
https://doi.org/10.1360/n972018-00099
https://doi.org/10.1360/n972018-00099
We explore the properties of nuclear pasta appearing in supernova matter, i.e., matter at finite temperature with a fixed proton fraction. The pasta phases with a series of geometric shapes are studied using the compressible liquid-drop (CLD) model,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::48af2cf4e43691f3b975f6c756c2b85c
Publikováno v:
Proceedings of the Workshop on Quarks and Compact Stars 2017 (QCS2017).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ddd8ea2c36a5dc021da3dd5e6b29a1b3
https://doi.org/10.7566/jpscp.20.011033
https://doi.org/10.7566/jpscp.20.011033
Publikováno v:
Physical Review C. 94
A self-consistent description for hot $\mathrm{\ensuremath{\Lambda}}$ hypernuclei in hypothetical big boxes is developed within the relativistic Thomas-Fermi approximation in order to investigate directly the liquid-gas phase coexistence in strangene
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e989381c0902a198df75593d0ecf4f9b
https://doi.org/10.1103/physrevc.94.054325
https://doi.org/10.1103/physrevc.94.054325
Autor:
Hong Shen, Shishao Bao
Publikováno v:
Physical Review C. 91
We study the impact of the symmetry energy on properties of nuclear pasta phases and crust-core transition in neutron stars. We perform a self-consistent Thomas-Fermi calculation employing the relativistic mean-field model. The properties of pasta ph
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::aecfc5683418d892ce20987323430367
https://doi.org/10.1103/physrevc.91.015807
https://doi.org/10.1103/physrevc.91.015807
Publikováno v:
Physical Review C. 90
We develop a self-consistent description of hot nuclei within the relativistic Thomas--Fermi approximation using the relativistic mean-field model for nuclear interactions. The temperature dependence of the symmetry energy and other physical quantiti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d1e69d4c921fc49b29ba030f1456cb9e
https://doi.org/10.1103/physrevc.90.054302
https://doi.org/10.1103/physrevc.90.054302
We study the effects of the symmetry energy on the neutron drip density and properties of nuclei in neutron star crusts. The nonuniform matter around the neutron drip point is calculated by using the Thomas--Fermi approximation with the relativistic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::81af116dff34329ee4b29e02fcdac67f
http://arxiv.org/abs/1410.0851
http://arxiv.org/abs/1410.0851