30 citations · 123 across the 9 of their papers we have counts for
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Properties of rapidly rotating hot neutron stars within Brueckner theory
Hong-Ming Liu, Bo-Xiu Zhou, Zeng-Hua Li +2
We study the properties of hot rapidly rotating neutron stars using various equations of state based on the Brueckner-Hartree-Fock approach at finite temperature. The temperature d…
Medium effects on neutron star modified and direct Urca cooling rates
B. X. Zhou, Jin-Biao Wei, Z. H. Li +2
We study the effects of in-medium modification of the elementary cooling processes on observable properties of isolated neutron stars. We then deduce the neutron star mass distribu…
Dark matter effects on the properties of neutron stars: compactness and tidal deformability
Hong-Ming Liu, Jin-Biao Wei, Zeng-Hua Li +3
We systematically study the observable properties of dark-matter admixed neutron stars, employing a realistic nuclear EOS in combination with self-interacting fermionic dark matter…
Dark matter effects on the properties of neutron stars: optical radii
Hong-Ming Liu, Jin-Biao Wei, Zeng-Hua Li +2
We study the effects of dark matter on the properties of neutron stars by employing a DM-admixed model. The Brueckner-Hartree-Fock theory with realistic three-body forces and a gen…
Non-radial oscillations and gravitational wave emission of hybrid neutron stars
Zi-Yue Zheng, Ting-Ting Sun, Huan Chen +3
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…
Microscopic nuclear equation of state at finite temperature and stellar stability
Hong-Ming Liu, Jing Zhang, Zeng-Hua Li +3
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…
Hot neutron stars and their equation of state
Jin-Biao Wei, G. F. Burgio, Ad. R. Raduta +1
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 fini…
Nuclear Pairing Gaps and Neutron Star Cooling
Jin-Biao Wei, Fiorella Burgio, Hans-Josef Schulze
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-Ha…
Constraints from the GW170817 merger event on the nuclear matter equation of state
G. F. Burgio, A. Figura, H. -J. Schulze +1
The detection of the GW170817 neutron star merger event has incited an intense research activity towards the understanding of the nuclear matter equation of state. In this paper we…