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2-7 Study of Zr-Nb Cycle in Astrophysical rp-process

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摘要 At a certain high temperature,this cycle will be dominant and end the rp-process to heavier region[2].It provides an upper temperature limit for rp-process along the proton drip line to produce nuclides beyond A=84,including the light p nuclides of 92;94Mo,96;94Ru.The existence of Zr-Nb cycle is an important question in rp-process[2].α-separation energy(Sα)of 84Mo plays an important role in the formation of this cycle.A strong enhancement of 83Nb(p,α)reaction rate is due to a very low Sαof 84Mo[1].
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出处 《IMP & HIRFL Annual Report》 2016年第1期40-41,共2页 中国科学院近代物理研究所和兰州重离子研究装置年报(英文版)
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