# name
Equation of state for neutron star calculations

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Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Xavier Viñas Gausí

# metadata.dc.description.abstract[].value
Neutron star matter is composed of neutrons, protons and electrons in a state of charge neutrality and β-equilibrium. In order to study the equation of state of this type of stellar matter, a zero-range type of nucleon-nucleon effective interactions, called Skyrme interactions, will be used within the Hartree-Fock approach. We also study the relation between the mass and the radius of neutron stars by solving the Tolman-Oppenheimer-Volkoff equations using the equation of state of neutron star matter.

# metadata.dc.title[].value
Equation of state for neutron star calculations