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Formation of Neutron-Rich and Superheavy Elements in Astrophysical Objects
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作者 rabinarayan panda Suresh Kumar Patra 《Journal of Modern Physics》 2010年第5期312-318,共7页
We calculate the reaction and the fusion cross-sections of neutron-rich heavy nuclei taking light exotic isotopes as projectiles. Results of neutron-rich Pb and U isotopes are demonstrated as the representative target... We calculate the reaction and the fusion cross-sections of neutron-rich heavy nuclei taking light exotic isotopes as projectiles. Results of neutron-rich Pb and U isotopes are demonstrated as the representative targets and He, B as the projectiles. The Gluaber Model and the Coupled Channel Formalism are used to evaluate the reaction and the fusion cross-sections for the cases considered. Based on the analysis of these cross-sections, we predict the formation of heavy, superheavy and super-superheavy elements through rapid neutron/ light nuclei capture r-process of the nucleosynthesis in astrophysical objects. 展开更多
关键词 Total NUCLEAR CROSS SECTION Fusion Reaction CROSS SECTION Gluaber Model Coupled Channel FORMALISM
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