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Stationary, Axisymmetric Neutron Stars with Meridional Circulation in General Relativity
Stationary Axisymmetric Neutron Stars Meridional Circulation General Relativity
2010/12/20
We present the first stationary, axisymmetric neutron star models with meridional circulation in general relativity. For that purpose, we developed GRNS, a new code based on a fixed point iteration.
Energy of Gravitational Field of Static Spherically Symmetric
Neutron Stars
the energy of gravitational field neutron star
Einstein-Tolman
expression
2007/8/15
2003Vol.40No.5pp.637-640DOI:
Energy of Gravitational Field of Static Spherically Symmetric
Neutron Stars
WEN De-Hua,1,2 CHEN Wei,3 WANG Xian-Ju,1
AI Bao-Quan,1 LIU Guo-Tao,1 and...
Properties of Rotating Neutron Stars in the Relativistic
σ-ω Model
relativistic σ-ω
model rotating neutron star equation of state
2007/8/15
2004Vol.41No.1pp.51-54DOI:
Properties of Rotating Neutron Stars in the Relativistic
σ-ω Model
WEN De-Hua,1,2 CHEN
Wei,3 WANG
Xian-Ju,1
AI Bao-Quan,1 LIU
Guo-Tao,1 and LIU
Lian...