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Tkachenko modes in rotating neutron stars: the effect of compressibility and implications for pulsar timing noise
Tkachenko modes rotating neutron stars effect of compressibility implications pulsar timing noise
2010/12/21
Long wavelength oscillations (Tkachenko waves) of the triangular lattice of quantized vortices in super uid neutron stars have been suggested as one of the possible explanations for the timing noise o...
Evolutions of Magnetized and Rotating Neutron Stars
Rotating Neutron Stars Evolutions of Magnetized
2010/3/17
We study the evolution of magnetized and rigidly rotating neutron stars within a fully general relativistic implementation of ideal magnetohydrodynamics with no assumed symmetries in three spatial dim...
Structure of Rotating Neutron Stars in Uniform Strong Magnetic Field
structure neutron star strong magnetic field
2007/8/15
2007Vol.47No.4pp.653-657DOI:
Structure of Rotating Neutron Stars in Uniform Strong Magnetic Field
WEN De-Hua,1 CHEN Wei,2 and LIU Liang-Gang3
1 Department of Physics, So...
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...