Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Jin-Biao Wei"'
Publikováno v:
Symmetry, Vol 16, Iss 7, p 807 (2024)
We investigate the equilibrium structure and radial oscillations of strange quark stars admixed with fermionic dark matter. For strange quark matter, we employ a stiff equation of state from a color-superconductivity improved bag model. For dark matt
Externí odkaz:
https://doaj.org/article/9f5ad2a15ec24b969b4120577cbbb8f1
Publikováno v:
Symmetry, Vol 13, Iss 3, p 400 (2021)
Background: We analyze several constraints on the nuclear equation of state (EOS) currently available from neutron star (NS) observations and laboratory experiments and study the existence of possible correlations among properties of nuclear matter a
Externí odkaz:
https://doaj.org/article/20e4aa146ef94b0fb08a43355dce9704
Publikováno v:
Universe, Vol 6, Iss 8, p 115 (2020)
We study the cooling of isolated neutron stars with particular regard to the importance of nuclear pairing gaps. A microscopic nuclear equation of state derived in the Brueckner-Hartree-Fock approach is used together with compatible neutron and proto
Externí odkaz:
https://doaj.org/article/2770861c154a4dd1b8c0f9554055bee1
We investigate non-radial oscillations of pure and hybrid neutron stars, employing equations of state of nuclear matter from Brueckner-Hartree-Fock theory, and of quark matter from the Dyson-Schwinger quark model, performing a Gibbs construction for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::11ee4f366b03acfa08cc44745e789f15
A microscopic nuclear equation of state compatible with all current astrophysical constraints constructed within the Brueckner-Hartree-Fock formalism is presented and extended in a consistent way to finite temperature. The effects of finite temperatu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2043e6c7b61a0b089e837c1407f3d44
http://arxiv.org/abs/2207.12146
http://arxiv.org/abs/2207.12146
Publikováno v:
Physical Review C. 104
A set of microscopic, covariant density-functional, and non-relativistic Skyrme-type equations of state is employed to study the structure of purely nucleonic neutron stars at finite temperature. After examining the agreement with presently available
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1536225319bbaa759c42bc29bdcc3dd8
https://doi.org/10.1103/physrevc.104.065806
https://doi.org/10.1103/physrevc.104.065806
Publikováno v:
Symmetry, Vol 13, Iss 400, p 400 (2021)
Symmetry
Volume 13
Issue 3
Symmetry
Volume 13
Issue 3
Background: We analyze several constraints on the nuclear equation of state (EOS) currently available from neutron star (NS) observations and laboratory experiments and study the existence of possible correlations among properties of nuclear matter a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::801abb236d5f2b61152a81fe35c6331c
https://www.mdpi.com/2073-8994/13/3/400
https://www.mdpi.com/2073-8994/13/3/400
Publikováno v:
Proceedings of XIII Quark Confinement and the Hadron Spectrum — PoS(Confinement2018).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d102ede59ef51d732c937879ca5b5201
https://doi.org/10.22323/1.336.0203
https://doi.org/10.22323/1.336.0203
Publikováno v:
2012 20th International Conference on Geoinformatics; 1/ 1/2012, p1-6, 6p