Equation of state for neutron star calculations

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dc.contributor.advisorViñas Gausí, Xavier
dc.contributor.authorVives Morell, Raquel
dc.date.accessioned2021-04-27T13:33:47Z
dc.date.available2021-04-27T13:33:47Z
dc.date.issued2020-01
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Xavier Viñas Gausíca
dc.description.abstractNeutron 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.ca
dc.format.extent5 p.
dc.format.mimetypeapplication/pdf
dc.identifier.urihttps://hdl.handle.net/2445/176778
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Vives, 2020
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.sourceTreballs Finals de Grau (TFG) - Física
dc.subject.classificationEstels de neutronscat
dc.subject.classificationEquacions d'estatcat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherNeutron starseng
dc.subject.otherEquations of stateeng
dc.subject.otherBachelor's theseseng
dc.titleEquation of state for neutron star calculationseng
dc.typeinfo:eu-repo/semantics/bachelorThesisca

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Treballs Finals de Grau (TFG) - Física