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Scientists have shown how gravitational waves—invisible ripples in the fabric of space and time that propagate through the universe—might be “seen” by looking at the stars. The new model, developed in...
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...