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Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutora: Àngels Ramos Gomez

# metadata.dc.description.abstract[].value
On 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.