Gravitational waves from a neutron star merger

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dc.contributor.advisorCentelles Aixalà, Mario
dc.contributor.authorBergonyó Forcades, Roger
dc.date.accessioned2020-09-30T14:23:00Z
dc.date.available2020-09-30T14:23:00Z
dc.date.issued2020-06
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Mario Centelles Aixalàca
dc.description.abstractIn this work we present the equations that describe the structure of neutron stars, as well as different models that describe the properties of the neutron star matter, using Skyrme nuclear interactions. From the data obtained in the gravitational waves detected in recent years we determine which models are still valid to describe the neutron star matter and which are not.ca
dc.format.extent5 p.
dc.format.mimetypeapplication/pdf
dc.identifier.urihttps://hdl.handle.net/2445/170971
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Bergonyó, 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.classificationOnes gravitacionalscat
dc.subject.classificationEstels de neutronscat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherGravitational waveseng
dc.subject.otherNeutron starseng
dc.subject.otherBachelor's theseseng
dc.titleGravitational waves from a neutron star mergereng
dc.typeinfo:eu-repo/semantics/bachelorThesisca

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Treballs Finals de Grau (TFG) - Física