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Chin. Phys. B, 2010, Vol. 19(9): 099601    DOI: 10.1088/1674-1056/19/9/099601
GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS Prev   Next  

Effect of superstrong magnetic field on electron screening at the crusts of neutron stars

Liu Jing-Jing
College of Science and Tecnology, Qiongzhou University, Sanya 572022, China
Abstract  The influences of electron screening (ES) and electron energy correction (EEC) are investigated by superstrong magnetic field (SMF). We also discuss in detail the discrepant factor between our results and those of Fushiki, Gudmundsson and Pethick (FGP) in SMF. The results show that SMF has only a slight effect on ES when B < 109 T on the surfaces of most neutron stars. Whereas for some magnetars, SMF influence ES greatly when B > 109 T . For instance, due to SMF the ES potential may be increased about 23.6% and the EEC may be increased about 4 orders of magnitude at ρ/μe = 1.0×106 mol/cm3 and T9 = 1. On the other hand, the discrepant factor shows that our results are in good agreement with FGP's when B < 109 T . But the difference will be increased with increasing SMF.
Keywords:  electron screening      superstrong magnetic field      neutron star     
Received:  07 September 2009      Published:  15 September 2010
PACS:  9635P  
  9760J  
Fund: Project supported by the Natural Science Foundation of Hainan Province, China (Grant No. 109004), the Scientific Research and Foundation of Hainan Provincial Education Department, China (Grant No. Hjkj2010-42) and the Special Foundation of Institutions for Higher Education of Sanya (Grant No. YD09047).

Cite this article: 

Liu Jing-Jing Effect of superstrong magnetic field on electron screening at the crusts of neutron stars 2010 Chin. Phys. B 19 099601

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