Viñas Gausí, XavierVives Morell, Raquel2021-04-272021-04-272020-01https://hdl.handle.net/2445/176778Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Xavier Viñas GausíNeutron star matter is composed of neutrons, protons and electrons in a state of charge neutrality and β-equilibrium. In order to study the equation of state of this type of stellar matter, a zero-range type of nucleon-nucleon effective interactions, called Skyrme interactions, will be used within the Hartree-Fock approach. We also study the relation between the mass and the radius of neutron stars by solving the Tolman-Oppenheimer-Volkoff equations using the equation of state of neutron star matter.5 p.application/pdfengcc-by-nc-nd (c) Vives, 2020http://creativecommons.org/licenses/by-nc-nd/3.0/es/Estels de neutronsEquacions d'estatTreballs de fi de grauNeutron starsEquations of stateBachelor's thesesinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/openAccess