# name
Calculation of the equation of state of neutron star matter

# metadata.dc.description[].value
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2023, Tutor: Mario Centelles Aixalà

# metadata.dc.description.abstract[].value
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.

# metadata.dc.title[].value
Calculation of the equation of state of neutron star matter