Rana, Shilpa and Kumar, Raj and Bhuyan, Mrutunjaya (2021) Fusion dynamics of 12 C + 12 C reaction: An astrophysical interest within the relativistic mean‐field approach. Astronomische Nachrichten, 342 (1-2). pp. 473-477. ISSN 0004-6337, DOI https://doi.org/10.1002/asna.202113953.
Full text not available from this repository.Abstract
The C-12 + C-12 fusion reaction plays a significant role in the later phases of stellar evolution. For a better understanding of the evolution involved, one must understand the corresponding fusion-fission dynamics and reaction characteristics. In the present analysis, we have studied the fusion cross-section along with the S-factor for this reaction using the well-known M3Y and recently developed R3Y nucleon-nucleon (NN) potential along with the relativistic mean-field densities in double-folding approach. The density distributions and the microscopic R3Y NN potential are calculated using the NL3* parameter set. The l- summed Wong model is employed to investigate the fusion cross-section, with l(max)-values from the sharp cut-off model. The calculated results are also then compared with the experimental data. It is found that the R3Y interaction gives a reasonable agreement with the data.
| Item Type: | Article |
|---|---|
| Funders: | Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Department of Atomic Energy (DAE), Board of Research in Nuclear Sciences (BRNS), FOSTECT |
| Uncontrolled Keywords: | Relativistic mean field; Nucleon‐; Nucleon potential; nucleus‐; Nucleus potential; Summed Wong model; Fusion cross‐ |
| Subjects: | Q Science > Q Science (General) Q Science > QB Astronomy Q Science > QC Physics |
| Divisions: | Faculty of Science |
| Depositing User: | Ms. Juhaida Abd Rahim |
| Date Deposited: | 18 Feb 2022 07:21 |
| Last Modified: | 18 Feb 2022 07:21 |
| URI: | http://eprints.um.edu.my/id/eprint/26274 |
Actions (login required)
 |
View Item |
