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I show that the usual model of the rotational response of a neutron star, which predicts rotation-induced neutronic vortices and no rotation-induced protonic vortices, does not hold (i) beyond a certa...
Neutron star crustal matter, whose properties are relevant in many models aimed at explaining observed astrophysical phenomena, has so far always been studied using a mean field approach. In order to ...
The connection between the radio emission from “lightnings” produced by the absorption of high-energy photons from the cosmic gamma-ray background in a neutron star magnetosphere and radio bursts from...
Motivated by an open question raised in recent times regarding the phase transition during the collapse of a neutron star to form a black hole and related stability issues, we have constructed charged...
We present a novel method to study the dynamics of bulk fermion systems such as the neutron- star crust. By introducing periodic boundary conditions into Fermionic Molecular Dynamics, it becomes pos...
We propose that the recently observed cooling of the neutron star in Cassiopeia A is due to enhanced neutrino emission from the onset of the breaking and formation of neutron Cooper pairs in the 3P2...
We present new results from accurate and fully general-relativistic simulations of the coalescence of unmagnetized binary neutron stars with various mass ratios. The evolution of the stars is followed...
Critical phenomena in gravitational collapse opened a new mathematical vista into the theory of general relativity and may ultimately entail fundamental physical implication in observations. However, ...
We study the influence of strong magnetic fields on antikaon condensation in neutron star matter using the quark-meson coupling (QMC) model. The QMC model describes a nuclear many-body system as nonov...
2001Vol.36No.3pp.327-330DOI: The Properties of Pure Neutron Star CHEN Wei,1 LI Quan-Guo2 and LIU Liang-Gang1 1 Department of Physics, Zhongshan University, Guangzhou 510...
2006Vol.45No.5pp.853-857DOI: Structural and Spacial Characters of Neutron Star in Relativistic σ-ω Model WEN De-Hua,1,2 HU Jian-Xun,1 and LIU Liang-Gang3 1 Department o...
2006Vol.45No.3pp.505-510DOI: Influence of Model Parameters on Hadron-Quark Phase Transition in Neutron Star Matter BAO Tmurbagan,1,2 LIU Guang-Zhou,1 and ZHU Ming-Feng1 ...
2003Vol.39No.4pp.439-446DOI: Three-Body Force Effects on EOS of Asymmetric Nuclear Matter and Proton Fraction in Neutron Star Matter ZUO Wei,1 A. Lejeune,2 U. Lombardo,3 and J.F. ...
2005Vol.43No.6pp.1042-1044DOI: Acceleration Effect in the Field of Neutron Star with Electric and Magnetic Charge and Magnetic Moment HE Tang-Mei and WANG Yong-Jiu Insti...
2005Vol.43No.4pp.704-708DOI: Neutron Star Magnetic Field as for Nonzero Photon Mass WANG Qing-Wu1 and LÜ Xiao-Fu1,2,3 1 Department of Physics, Sichuan University, C...

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