# metadata.dc.description[].value
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutor: Mario Centelles Aixalà

# metadata.dc.description.abstract[].value
A study on neutron stars, regarding the equations of state and the structure equations used to model them, has been performed as a benchmark for investigating the tidal deformability of these compact stars, which may be accessed through gravitational wave detections, and its contribu-tion in obtaining generic (model-independent) relations between neutron star relevant magnitudes.