Centelles Aixalà, MarioHernández Toledo, Adrià2023-07-252023-07-252023-06https://hdl.handle.net/2445/201118Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2023, Tutor: Mario Centelles AixalàSymmetric 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.5 p.application/pdfengcc-by-nc-nd (c) Hernández, 2023http://creativecommons.org/licenses/by-nc-nd/3.0/es/Equació d'estatEstels de neutronsTreballs de fi de grauEquation of stateNeutron starsBachelor's thesesinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/openAccess