1. Dipòsit Digital de la Universitat de Barcelona
  2. Treballs de l'alumnat
  3. Treballs Finals de Grau (TFG) - Física
Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/170971
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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.identifier.urihttp://hdl.handle.net/2445/170971-
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.language.isoengca
dc.rightscc-by-nc-nd (c) Bergonyó, 2020-
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
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
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