搜索结果: 1-13 共查到“理论物理学 stars”相关记录13条 . 查询时间(0.14 秒)
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...
Energy release from hadron-quark phase transition in neutron stars and the axial $w$-mode of gravitational waves
Energy release hadron-quark phase transition axial $w$-mode of gravitational waves
2010/12/21
Describing the hyperonic and quark phases of neutron stars with an isospin- and momentum-
dependent effective interaction for the baryon octet and the MIT bag model, respectively, and using the Gibbs...
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.
Gravitational Waves from the $r$-mode instability of neutron stars: effect of magnetic field
Gravitational Waves $r$-mode instability neutron stars: effect magnetic field
2010/12/20
Studies have shown that emission of gravitational waves drives an instability in the r-modes
of young rapidly rotating neutron stars carrying away most of the angular momentum through
gravitational ...
Neutrino energy loss by electron capture in magnetic field at the crusts of neutron stars
strong magnetic field neutrino energy loss neutron star
2009/7/31
Based on the p-f shell model, the effect of strong magnetic field on neutrino energy loss rates by electron capture is investigated. The calculations show that the magnetic field has only a slight eff...
The Effect of Hyperon-Hyperon Interaction on Neutron Stars
neutron star matter relativistic mean-field approximation
hyperon-hyperon interaction
2007/8/15
2001Vol.36No.4pp.446-448DOI:
The Effect of Hyperon-Hyperon Interaction on Neutron Stars
SUN Bao-Xi,1,2,3 JIA Huan-Yu,3 MENG Jie2,3,4 and
ZHAO En-Guang2,4
1 Institute of ...
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...
Magnetic Field Effect on
β+ Decay in the Crusts of
Accreting Neutron Stars
β+ decay strong magnetic field neutron star
2007/8/15
2007Vol.47No.4pp.765-768DOI:
Magnetic Field Effect on
β+ Decay in the Crusts of
Accreting Neutron Stars
ZHANG Jie, LIU Men-Quan, and LUO Zhi-Quan
Institute of Physics ...
Antikaon Condensation and In-medium Kaon and Antikaon
Production in Protoneutron Stars
protoneutron stars antikaon condensation neutrino trapping
2007/8/15
2007Vol.47No.1pp.111-118DOI:
Antikaon Condensation and In-medium Kaon and Antikaon
Production in Protoneutron Stars
GU Jian-Fa,1 GUO Hua,1,2 LI Xi-Guo,2,3 LIU Yu-Xin,1,2,4 and XU ...
Gravitomagnetic Effects on Collective Plasma Oscillations in Compact Stars
gravitomagnetism compact stars plasma osillations
2007/8/15
2006Vol.45No.3pp.568-572DOI:
Gravitomagnetic Effects on Collective Plasma Oscillations in Compact Stars
Babur M. Mirza1 and Hamid Saleem2,3
1 Department of Mathematics, ...
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...
Neutron Stars in the Model of Non-linear Realization of
SU(2) Chiral Symmetry Spontaneous Breaking
neutron star chiral symmetry spontaneous breaking relativistic
mean-field approximation
2007/8/15
2003Vol.39No.5pp.603-606DOI:
Neutron Stars in the Model of Non-linear Realization of
SU(2) Chiral Symmetry Spontaneous Breaking
WANG Nan,2 SUN Bao-Xi,1 LÜ Xiao-Fu,2,3
and ZH...
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...