中国物理B ›› 2006, Vol. 15 ›› Issue (7): 1477-1480.doi: 10.1088/1009-1963/15/7/016
张洁, 刘门全, 罗志全
Zhang Jie (张洁), Liu Men-Quan (刘门全), Luo Zhi-Quan (罗志全)
摘要: βdecay in the strong magnetic field of the crusts of neutron stars is analysed by an improved method. The reactions 67 Ni(β-)67 Cu and 62 Mn\beta -62 Fe are investigated as examples. The results show that a weak magnetic field has little effect on βdecay but a strong magnetic field (B>1012G) increases β decay rates obviously. The conclusion derived may be crucial to the research of late evolution of neutron stars and nucleosynthesis in r-process.
中图分类号: (Neutron stars)