Chin. Phys. Lett.  2007, Vol. 24 Issue (3): 628-631    DOI:
Original Articles |
Properties of Neutron Stars Rotating at Kepler Frequency with Uniform Strong Magnetic Field

WEN De-Hua1;CHEN Wei2;LU Yi-Gang1;LIU Liang-Gang3

1School of Physics, South China University of Technology, Guangzhou 5106412Department of Physics, Jinan University, Guangzhou 5106323The Faculty of Information Technology, Macau University of Science and Technology, Macao
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WEN De-Hua, CHEN Wei, LU Yi-Gang et al  2007 Chin. Phys. Lett. 24 628-631
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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.
Keywords: 04.40.Dg      95.30.Sf      97.10.Kc      97.60.Jd     
Received: 11 August 2006      Published: 08 February 2007
PACS:  04.40.Dg (Relativistic stars: structure, stability, and oscillations)  
  95.30.Sf (Relativity and gravitation)  
  97.10.Kc (Stellar rotation)  
  97.60.Jd (Neutron stars)  
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https://cpl.iphy.ac.cn/       OR      https://cpl.iphy.ac.cn/Y2007/V24/I3/0628
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WEN De-Hua
CHEN Wei
LU Yi-Gang
LIU Liang-Gang
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