Ramos Gómez, ÀngelsGimeno Estivill, Patrícia2021-09-282021-09-282021-02https://hdl.handle.net/2445/180306Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutora: Àngels Ramos GomezOn 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.5 p.application/pdfengcc-by-nc-nd (c) Gimeno, 2021http://creativecommons.org/licenses/by-nc-nd/3.0/es/Estels de neutronsOnes gravitacionalsTreballs de fi de grauNeutron starsGravitational wavesBachelor's thesesinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/openAccess