Mean-field description of heavy-ion scattering at low energies and fusion
Mean-field description of heavy-ion scattering at low energies and fusion作者机构:Institute for Nuclear Science and Technology VINATOM Department of Nuclear Physics and Nuclear EngineeringFaculty of Physics and Engineering Physics University of Science VNU-HCM
出 版 物:《Nuclear Science and Techniques》 (核技术(英文))
年 卷 期:2018年第29卷第12期
页 面:102-111页
核心收录:
学科分类:080706[工学-化工过程机械] 08[工学] 0807[工学-动力工程及工程热物理] 0827[工学-核科学与技术] 082701[工学-核能科学与工程]
基 金:supported in part by the National Foundation for Scientific and Technological Development(NAFOSTED Project No.103.04-2017.317)
主 题:精力 熔化 散布 重离子 状态密度 密度依赖 相互作用 天体物理学
摘 要:The nuclear mean-field potential built up during the ^(12)C+^(12)C and ^(16)O+^(16)O collisions at low energies relevant for the carbon-and oxygen-burning processes is constructed within the double-folding model(DFM) using the realistic ground-state densities of^(12)C and^(16)O, and CDM3Yn density-dependent nucleon–nucleon(NN) interaction. The rearrangement term, indicated by the Hugenholtz–van Hove theorem for the single-particle energy in nuclear matter, is properly considered in the DFM calculation. To validate the use of the density-dependent NN interaction at low energies, an adiabatic approximation was suggested for the dinuclear overlap density. The reliability of the nucleus–nucleus potential predicted through this low-energy version of the DFM was tested in the optical model(OM) analysis of the elastic^(12)C+^(12)C and ^(16)O+^(16)O scattering data at energies below 10 MeV/*** OM results provide a consistently good description of the elastic angular distributions and 90 excitation function. The dinuclear mean-field potential predicted by the DFM is further used to determine the astrophysical S factor of the ^(12)C+^(12)C and ^(16)O+^(16)O fusions in the barrier penetration model. Without any adjustment of the potential strength, our results reproduce the non-resonant behavior of the S factor of the ^(12)C+^(12)C and ^(16)O+^(16)O fusions very well over a wide range of energies.