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作 者:Lam Yihua He Jianjun Parikh Anuj
机构地区:[1]不详 [2]Departament de F待sica i Enginyeria Nuclear, Universitat Politecnica de Catalunya (EUETIB), E-08036 Barcelona, Spain
出 处:《IMP & HIRFL Annual Report》2014年第1期48-49,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)
基 金:Auspices of Ministry of Science and Technology of China (Talented Young Scientist Program), China PostdoctoralScience Foundation (2014M562481).
摘 要:We have derived new thermonuclear 64Ge(p, )65As and 65As(p, )66Se reaction rates based on recently evaluatedproton separation energies[1] and large-scale shell model (LSSM) calculation. The precisely measured or evaluatedproton separation energies of Sp(65As) and Sp(66Se), are (90±85) keV and (1720±310) keV, respectively. Weutilized one-zone post-processing type I X-ray burst model[2] to investigate the astrophysical impact of our newrates. We found that the new experimental Sp(65As), resonant energies and spectroscopic factors estimated fromLSSM significantly affects the productions of nuclide in the range of 64≤A≤110 about one to ten times comparedto currently available JINA data sets, REACLIB[3].
关 键 词:X-RAY experimental impact RANGE TIMES SETS OUR
分 类 号:TP31[自动化与计算机技术—计算机软件与理论]
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