6th Nuclear Physics in Astrophysics | |
12C+12C fusion in a multichannel folding model | |
物理学;天文学 | |
Assunção, M.^1 ; Descouvemont, P.^2 | |
Departamento de Ciências Exatas e da Terra, Universidade Federal de São Paulo, Campus Diadema, São Paulo | |
09972-270, Brazil^1 | |
Physique Nucléaire Théorique et Physique Mathématique, Université Libre de Bruxelles (ULB), C.P. 229, Brussels | |
B 1050, Belgium^2 | |
关键词: Coulomb barrier; Coupled channels; Density dependent; Fitting parameters; Folding modeling; Nucleon-nucleon interaction; Optical potential; Transition density; | |
Others : https://iopscience.iop.org/article/10.1088/1742-6596/665/1/012010/pdf DOI : 10.1088/1742-6596/665/1/012010 |
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学科分类:天文学(综合) | |
来源: IOP | |
【 摘 要 】
The12C+12C fusion reaction is investigated using a folding potential in a multichannel approach involving the12C(0+1, 2+, 0+2, 3-) states. The12C densities (including transition densities) are taken from the RGM calculation of Kamimura. For the nucleon-nucleon interaction, we use the DDM3Y density-dependent interaction. Owing to the explicit presence of inelastic channels, the imaginary part of the optical potential only contains a short-range fusion contribution. The S-factor is then virtually insensitive to the precise value, and the model is free of any fitting parameter. From the coupled-channel system, we determine the elastic and fusion cross sections simultaneously. As elastic data are available around the Coulomb barrier, this simultaneous treatment offers a good test for the reliability of the model. In the fusion cross section, the role of the inelastic channels and, in particular of the12C(0+1)+12C(0+2) channel involving the Hoyle state, is discussed.
【 预 览 】
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