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Beta decay of nuclides ^(56)Fe,^(62)Ni,^(64)Ni and ^(68)Ni in the crust of magnetars
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作者 Jing-Jing Liu Xiao-Ping Kang +4 位作者 Liang-Huan Hao Hao Feng Dong-Mei Liu Chang-Wei Li Xiang-Ming Zeng 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2016年第11期71-80,共10页
By introducing the Dirac δ-function and Pauli exclusion principle in the presence of superstrong magnetic fields (SMFs), we investigate the influence of SMFs on beta decay and the change rates of electron fraction ... By introducing the Dirac δ-function and Pauli exclusion principle in the presence of superstrong magnetic fields (SMFs), we investigate the influence of SMFs on beta decay and the change rates of electron fraction (CREF) of nuclides 56Fe, 62Ni, 64Ni and 6SNi in magnetars, which are powered by magnetic field energy. We find that the magnetic fields have a great influence on the beta decay rates, and the beta decay rates can decrease by more than six orders of magnitude in the presence of SMFs. The CREF also decreases by more than seven orders of magnitude in the presence of SMFs. 展开更多
关键词 physical data and processes: nuclear reactions NUCLEOSYNTHESIS abundances -- stars: neutron-- stars: magnetic fields
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Strong screening effects on resonant nuclear reaction ^(23)Mg(p,γ) ^(24)Al in the surface of magnetars
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作者 Jing-Jing Liu 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2016年第5期117-124,共8页
Based on the theory of relativistic superstrong magnetic fields (SMFs), by using the method of Thomas-Fermi-Dirac approximations, we investigate the problem of strong electron screening (SES) in SMFs and the influ... Based on the theory of relativistic superstrong magnetic fields (SMFs), by using the method of Thomas-Fermi-Dirac approximations, we investigate the problem of strong electron screening (SES) in SMFs and the influence of SES on the nuclear reaction of 23Mg (p, Y)24A1. Our calculations show that the nuclear reaction will be markedly effected by the SES in SMFs in the surface of magnetars. Our calculated screening rates can increase two orders of magnitude due to SES in SMFs. 展开更多
关键词 physical data and processes: nuclear reactions NUCLEOSYNTHESIS abundances -- stars: neutron-- stars: magnetic fields
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强磁场中修正URCA过程的中微子产能率 被引量:4
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作者 张洁 刘门全 +1 位作者 魏丙涛 罗志全 《物理学报》 SCIE EI CAS CSCD 北大核心 2008年第9期5448-5451,共4页
基于n-p-e模型并考虑修正URCA过程中的质子分支,研究了强磁场对中子星核心区域修正URCA过程中微子产能率的影响.结果表明,强磁场使修正URCA过程的中微子产能率产生明显振荡;与中子分支相比,强磁场对质子分支中微子产能率的影响偏弱,但... 基于n-p-e模型并考虑修正URCA过程中的质子分支,研究了强磁场对中子星核心区域修正URCA过程中微子产能率的影响.结果表明,强磁场使修正URCA过程的中微子产能率产生明显振荡;与中子分支相比,强磁场对质子分支中微子产能率的影响偏弱,但是它将提高总的中微子产能率.所得结论将有助于进一步研究中子星的冷却机理. 展开更多
关键词 中子星 强磁场 修正的urca过程
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