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.
| Authors: | , |
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| Format: | article |
| Status: | Published version |
| Publication Date: | 1981 |
| Country: | España |
| Institution: | Universidad de Barcelona |
| Repository: | Dipòsit Digital de la UB |
| OAI Identifier: | oai:diposit.ub.edu:2445/12235 |
| Online Access: | https://hdl.handle.net/2445/12235 |
| Access Level: | Open access |
| Keyword: | Estructura nuclear Astrofísica nuclear Ecuacions d'estat Nuclear structure Nuclear astrophysics Equations of state |
| Summary: | The properties of hot, dense stellar matter are investigated with a finite temperature nuclear Thomas-Fermi model. |
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