| Texto completo | |
| Autor(es): |
Kumar, Ankit
;
Das, H. C.
;
Kaur, Manpreet
;
Bhuyan, M.
;
Patra, S. K.
Número total de Autores: 5
|
| Tipo de documento: | Artigo Científico |
| Fonte: | PHYSICAL REVIEW C; v. 103, n. 2, p. 8-pg., 2021-02-02. |
| Resumo | |
We obtained a density-dependent analytical expression of binding energy per nucleon for different neutron- proton asymmetry of the nuclear matter (NM) with a polynomial fitting, which manifests the results of effective- field theory motivated relativistic mean-field (E-RMF) model. This expression has the edge over the Bruckner energy density functional [Phys. Rev. 171, 1188 (1968)] since it resolves the Coster-Band problem. The NM parameters like incompressibility, neutron pressure, symmetry energy, and its derivatives are calculated using the acquired expression of energy per nucleon. Furthermore, the weight function calculated by E-RMF densities are folded with calculated NM parameters within coherent density fluctuation model to find the properties of closed or semiclosed-shell even-even O-16, Ca-40, Ca-48, Ni-56 , Zr-90, (116 )n, and Pb-208 nuclei. The values obtained for the neutron pressure P-A, symmetry energy S-A , and its derivative L(sym)( )(A)known as the slope parameter lie within a narrow domain whereas there is a large variation in isoscalar incompressibility K-A and surface incompressibility K-sym(A) while moving from light to heavy nuclei. The sizable variation in K-A and K-sym(A) for light and heavy nuclei depicts their structural dependence due to the peculiar density distribution of each nucleus. A comparison of surface quantities calculated in the present work has also been made with ones obtained via Bruckner energy density functional. (AU) | |
| Processo FAPESP: | 17/05660-0 - Estudos teóricos da estrutura e reações de núcleos exóticos e sistemas de muitos corpos |
| Beneficiário: | Brett Vern Carlson |
| Modalidade de apoio: | Auxílio à Pesquisa - Temático |