Neutron Stars and Gravitational Waves

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dc.contributor.advisorRamos Gómez, Àngels
dc.contributor.authorGimeno Estivill, Patrícia
dc.date.accessioned2021-09-28T16:36:37Z
dc.date.available2021-09-28T16:36:37Z
dc.date.issued2021-02
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutora: Àngels Ramos Gomezca
dc.description.abstractOn the basis of a simple model for the energy of nuclear matter, we parametrize different equations of state within the constraints of experimental data to describe neutron stars with masses larger than 2M☉. Furthermore, we predict the dimensionless tidal deformability for a family of neutron stars characterized by the mass-radius relation computed from each equation of state. The obtained results are compared with recent observations of millisecond pulsars and gravitational-wave data to conclude with the choice of the best parametrized equation of state to describe the neutron stars observed.ca
dc.format.extent5 p.
dc.format.mimetypeapplication/pdf
dc.identifier.urihttps://hdl.handle.net/2445/180306
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Gimeno, 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.classificationOnes gravitacionalscat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherNeutron starseng
dc.subject.otherGravitational waveseng
dc.subject.otherBachelor's theseseng
dc.titleNeutron Stars and Gravitational Waveseng
dc.typeinfo:eu-repo/semantics/bachelorThesisca

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Treballs Finals de Grau (TFG) - Física