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

Neutrino energy loss by electron capture in magnetic field at the crusts of neutron stars
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摘要 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 10^8-10^13 G on the surfaces of most neutron stars. But for some magnetars, the range of the magnetic field is 10^13-10^18 G, and the neutrino energy loss rates are greatly reduced, even by more than four orders of magnitude due to the strong magnetic field. 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 10^8-10^13 G on the surfaces of most neutron stars. But for some magnetars, the range of the magnetic field is 10^13-10^18 G, and the neutrino energy loss rates are greatly reduced, even by more than four orders of magnitude due to the strong magnetic field.
出处 《Chinese Physics C》 SCIE CAS CSCD 北大核心 2008年第2期108-111,共4页 中国物理C(英文版)
基金 Supported by National Natural Science Foundation of China (10778719) Scientific Research and Fund of Sichuan Provincial Education Department (2006A079)
关键词 strong magnetic field neutrino energy loss neutron star strong magnetic field, neutrino energy loss, neutron star
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