55 citations · 230 across the 17 of their papers we have counts for
18 papers
Neutron star cooling with medium-modified Urca rates
B. X. Zhou, J. B. Wei, Jin-Biao Wei +3
We study the effects of in-medium modification of the elementary cooling processes on observable properties of isolated neutron stars. We deduce the neutron star mass distributions…
Two-fluid -mode oscillations of dark-matter-admixed neutron stars
Zi-Yue Zheng, Ting-Ting Sun, Huan Chen +4
We study quadrupolar -mode oscillations of dark-matter-admixed neutron stars (DANSs) in full general relativity (GR). The ordinary component is described by microscopic Brueckne…
Quasiradial oscillations of rotating hybrid neutron stars
Zi-Yue Zheng, Ting-Ting Sun, Huan Chen +4
We investigate fundamental quasiradial oscillations in slow-rotation approximation of pure and hybrid neutron stars, employing equations of state of nuclear matter from Brueckner-H…
Dark matter effects on the properties of hybrid neutron stars
Jin-Biao Wei, G. Wu, H. Chen +2
We study the effects of dark matter on the properties of hybrid neutron stars, in particular the influence on the mass-radius relation, the value of the maximum mass, and the hadro…
ESO Expanding Horizon White Paper: Revealing the properties of matter at supranuclear densities with gravitational waves
Tim Dietrich, Tanja Hinderer, Micaela Oertel +40
Understanding dense matter under extreme conditions is one of the most fundamental puzzles in modern physics. Complex interactions give rise to emergent, collective phenomena. Whil…
Cooling of dark neutron stars
B. X. Zhou, H. C. Das, J. B. Wei +3
We study the cooling of isolated dark-matter-admixed neutron stars, employing a realistic nuclear equation of state and realistic nuclear pairing gaps, together with fermionic dark…
Dense Matter in Neutron Stars with eXTP
Ang Li, Anna L. Watts, Guobao Zhang +82
In this White Paper, we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission to constrain the equation of state of dense matter in neutron stars, explo…
Neutron Decay Anomaly and Its Effects on Neutron Star Properties
H. C. Das, G. F. Burgio
We investigate the effects of dark matter (DM) on neutron star (NS) properties using the neutron decay anomaly model within the relativistic mean-field (RMF) framework. Three nucle…
-mode oscillations of protoneutron stars
Zi-Yue Zheng, Ting-Ting Sun, Huan Chen +4
We investigate nonradial -mode oscillations of protoneutron stars in full general relativity, employing equations of state described by the Brueckner-Hartree-Fock theory or the…
-mode oscillations of hybrid stars with pasta construction
Zi-Yue Zheng, Jin-Biao Wei, Huan Chen +3
We investigate nonradial -mode oscillations of hybrid neutron stars in full general relativity, employing hybrid equations of state describing a nuclear outer core and a pasta-p…
The nuclear symmetry energy and the neutron skin thickness in nuclei
G. F. Burgio, H. C. Das, I. Vidana
We investigate possible correlations between the stiffness of the symmetry energy at saturation density, the so-called parameter, and the neutron skin thickness of Ca…
Radial oscillations of proto-neutron stars
T. T. Sun, H. Chen, J. B. Wei +3
We investigate radial oscillations of proto-neutron stars, employing equations of state described by the Brueckner-Hartree-Fock theory or the relativistic mean field model, and ass…
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…
Neutron star cooling and mass distributions
H. C. Das, Jin-Biao Wei, G. F. Burgio +1
We study the cooling of isolated neutron stars, employing different nuclear equations of state with or without active direct Urca process, and investigate the interplay with the nu…
Binary neutron star merger simulations with hot microscopic equations of state
A. Figura, F. Li, J. -J. Lu +3
We perform binary neutron star merger simulations using a newly derived set of finite-temperature equations of state in the Brueckner-Hartree-Fock approach. We point out the import…
Hybrid equation of state approach in binary neutron-star merger simulations
A. Figura, J. -J. Lu, G. F. Burgio +2
We investigate the use of hybrid equations of state in binary neutron-star simulations in full general relativity, where thermal effects are included in an approximate way through…
Neutron star cooling with microscopic equations of state
J. -B. Wei, G. F. Burgio, H. -J. Schulze
We model neutron star cooling with several microscopic nuclear equations of state based on different nucleon-nucleon interactions and three-body forces, and compatible with the rec…
Thermal states of neutron stars with a consistent model of interior
M. Fortin, G. Taranto, G. F. Burgio +3
We model the thermal states of both isolated neutron stars and accreting neutron stars in X-ray transients in quiescence and confront them with observations. We use an equation of…