Equation of state of hot, dense stellar matter. Finite temperature nuclear Thomas-Fermi approach
The properties of hot, dense stellar matter are investigated with a finite temperature nuclear Thomas-Fermi model.
| Autores: | , |
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| Formato: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 1981 |
| País: | España |
| Recursos: | Universidad de Barcelona |
| Repositorio: | Dipòsit Digital de la UB |
| OAI Identifier: | oai:diposit.ub.edu:2445/12235 |
| Acesso em linha: | https://hdl.handle.net/2445/12235 |
| Access Level: | acceso abierto |
| Palavra-chave: | Estructura nuclear Astrofísica nuclear Ecuacions d'estat Nuclear structure Nuclear astrophysics Equations of state |
| Resumo: | The properties of hot, dense stellar matter are investigated with a finite temperature nuclear Thomas-Fermi model. |
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