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Title: Equation of state for neutron star calculations
Author: Vives Morell, Raquel
Director/Tutor: Viñas Gausí, Xavier
Keywords: Estels de neutrons
Equacions d'estat
Treballs de fi de grau
Neutron stars
Equations of state
Bachelor's thesis
Issue Date: Jan-2020
Abstract: 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.
Note: Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Xavier Viñas Gausí
Appears in Collections:Treballs Finals de Grau (TFG) - Física

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