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《中国物理C》(英文)编辑部
2024年10月30日

Neutrino energy loss by electron capture in magnetic field at the crusts of neutron stars

  • 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 effect on the neutrino energy loss rates in the range of 108—1013G on the surfaces of most neutron stars. But for some magnetars, the range of the magnetic field is 1013—1018G, and the neutrino energy loss rates are greatly reduced, even by more than four orders of magnitude due to the strong magnetic field.
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  • [1] . Fuller G M, Fowler W A, Newman M J. AP. J, 1980, 42:4472. Fuller G M, Fowler W A, Newman M J. AP. J, 1982, 252:7153. Fuller G M, Fowler W A, Newman M J. AP. J, 1982, 48:2794. Fuller G M, Fowler W A, Newman M J. AP. J, 1985, 293:15. Naoki Itoh, Akinori Nishikawa, Yasuharu Kohyama et al.AP. J, 1996, 470: 10156. Naoki Itoh, Hiroshi Hayashi, Akinori Nishikawa et al. AP.J, 1996, 102: 4117. Esposito S, Mangano G, Miele G et al. Nuclear Physics B,2003, 658: 2178. Indranath Bhattacharyya. J. Phys. G, 2006, 32: 9259. Dipankar Bhattachar Y A. Astro-ph, 2002, 23: 6710. Duan H Y, Qian Y Z. Astro-ph, 2005, 2: 7211. Goyal A, Gupta V K, Kanupriya et al. Int. J Mod. Phys.A, 2001, 16: 4712. Chakrabarty S. Int. J Mod. Phys. A, 1998, 13: 19513. Fushiki I, Gudmnndsson E H, Pethick C J. AP. J, 1989,342: 98514. Kiminker A D, Yakovlev D G. Theor. Math. Phys., 1981,49: 101215. Pruet J J, Fuller G M. AP. J. S., 2003, 149: 18916. Dai Z G, Lu T, Peng Q H. Astro Astrophys, 1993, 272:70517. Baym G, Pethick C. Ann J. Rev. Nucl. Sci., 1975, 25: 2718. LIU J J, LUO Z Q. Chinese Physics Lett., 2007, 7: 1861
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LIU Jing-Jing and LUO Zhi-Quan. Neutrino energy loss by electron capture in magnetic field at the crusts of neutron stars[J]. Chinese Physics C, 2008, 32(2): 108-111. doi: 10.1088/1674-1137/32/2/007
LIU Jing-Jing and LUO Zhi-Quan. Neutrino energy loss by electron capture in magnetic field at the crusts of neutron stars[J]. Chinese Physics C, 2008, 32(2): 108-111.  doi: 10.1088/1674-1137/32/2/007 shu
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Received: 2007-03-22
Revised: 2007-08-06
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Neutrino energy loss by electron capture in magnetic field at the crusts of neutron stars

    Corresponding author: LIU Jing-Jing,

Abstract: 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 effect on the neutrino energy loss rates in the range of 108—1013G on the surfaces of most neutron stars. But for some magnetars, the range of the magnetic field is 1013—1018G, and the neutrino energy loss rates are greatly reduced, even by more than four orders of magnitude due to the strong magnetic field.

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