Tidal Deformability of Neutron Stars

dc.contributor.advisorCentelles Aixalà, Mario
dc.contributor.authorMorell Ferrer, Pol
dc.date.accessioned2021-10-26T15:23:42Z
dc.date.available2021-10-26T15:23:42Z
dc.date.issued2021-07
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutor: Mario Centelles Aixalàca
dc.description.abstractA study on neutron stars, regarding the equations of state and the structure equations used to model them, has been performed as a benchmark for investigating the tidal deformability of these compact stars, which may be accessed through gravitational wave detections, and its contribu-tion in obtaining generic (model-independent) relations between neutron star relevant magnitudes.ca
dc.format.extent6 p.
dc.format.mimetypeapplication/pdf
dc.identifier.urihttps://hdl.handle.net/2445/180837
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Morell, 2021
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.titleTidal Deformability of Neutron Starseng
dc.typeinfo:eu-repo/semantics/bachelorThesisca

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