Properties of Neutron Stars Rotating at Kepler Frequency with Uniform Strong Magnetic Field
-
Abstract
A uniform strong magnetic field is considered in calculating the properties of neutron star rotating at the Kepler frequency. The results show that the effect of the magnetic field on the properties of neutron star is evident, and the properties of the neutron stars rotating at the Kepler frequency can be used as a criterion to the equations of states of the neutron star matters.
Article Text
-
-
-
About This Article
Cite this article:
WEN De-Hua, CHEN Wei, LU Yi-Gang, LIU Liang-Gang. Properties of Neutron Stars Rotating at Kepler Frequency with Uniform Strong Magnetic Field[J]. Chin. Phys. Lett., 2007, 24(3): 628-631.
WEN De-Hua, CHEN Wei, LU Yi-Gang, LIU Liang-Gang. Properties of Neutron Stars Rotating at Kepler Frequency with Uniform Strong Magnetic Field[J]. Chin. Phys. Lett., 2007, 24(3): 628-631.
|
WEN De-Hua, CHEN Wei, LU Yi-Gang, LIU Liang-Gang. Properties of Neutron Stars Rotating at Kepler Frequency with Uniform Strong Magnetic Field[J]. Chin. Phys. Lett., 2007, 24(3): 628-631.
WEN De-Hua, CHEN Wei, LU Yi-Gang, LIU Liang-Gang. Properties of Neutron Stars Rotating at Kepler Frequency with Uniform Strong Magnetic Field[J]. Chin. Phys. Lett., 2007, 24(3): 628-631.
|