Excitation energy dependence of the symmetry energy of finite nuclei
A finite-range density and momentum-dependent effective interaction is used to calculate the density and temperature dependence of the symmetry energy coefficient C{sub sym}({rho},T) of infinite nuclear matter. This symmetry energy is then used in the local density approximation to evaluate the exci...
| Autores: | , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2007 |
| País: | España |
| Institución: | Universidad de Barcelona |
| Repositorio: | Dipòsit Digital de la UB |
| OAI Identifier: | oai:diposit.ub.edu:2445/12208 |
| Acceso en línea: | https://hdl.handle.net/2445/12208 |
| Access Level: | acceso abierto |
| Palabra clave: | Reaccions nuclears Estructura nuclear Nuclear reactions Nuclear structure |
| Sumario: | A finite-range density and momentum-dependent effective interaction is used to calculate the density and temperature dependence of the symmetry energy coefficient C{sub sym}({rho},T) of infinite nuclear matter. This symmetry energy is then used in the local density approximation to evaluate the excitation energy dependence of the symmetry energy coefficient of finite nuclei in a microcanonical formulation that accounts for thermal and expansion effects. The results are in good harmony with the recently reported experimental data from energetic nucleus-nucleus collisions. |
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