Please use this identifier to cite or link to this item:
https://hdl.handle.net/2445/201118| Title: | Calculation of the equation of state of neutron star matter |
| Author: | Hernández Toledo, Adrià |
| Director/Tutor: | Centelles Aixalà, Mario |
| Keywords: | Equació d'estat Estels de neutrons Treballs de fi de grau Equation of state Neutron stars Bachelor's theses |
| Issue Date: | Jun-2023 |
| Abstract: | Symmetric nuclear matter, asymmetric nuclear matter and β-stable nuclear matter are discussed and modeled through a Lagrangian density of relativistic mean field (RMF) theory using a σ meson to describe the attractive interaction between nucleons, a ω meson to describe the repulsive interaction and a ρ meson to describe the asymmetry effects with the NL3 parametrization. |
| Note: | Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2023, Tutor: Mario Centelles Aixalà |
| URI: | https://hdl.handle.net/2445/201118 |
| Appears in Collections: | Treballs Finals de Grau (TFG) - Física |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| HERNANDEZ TOLEDO ADRIA_7934176.pdf | 435.98 kB | Adobe PDF | View/Open |
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