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DC Field | Value | Language |
---|---|---|
dc.contributor.advisor | Viñas Gausí, Xavier | - |
dc.contributor.author | Vives Morell, Raquel | - |
dc.date.accessioned | 2021-04-27T13:33:47Z | - |
dc.date.available | 2021-04-27T13:33:47Z | - |
dc.date.issued | 2020-01 | - |
dc.identifier.uri | http://hdl.handle.net/2445/176778 | - |
dc.description | Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Xavier Viñas Gausí | ca |
dc.description.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. | ca |
dc.format.extent | 5 p. | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | eng | ca |
dc.rights | cc-by-nc-nd (c) Vives, 2020 | - |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ | * |
dc.source | Treballs Finals de Grau (TFG) - Física | - |
dc.subject.classification | Estels de neutrons | cat |
dc.subject.classification | Equacions d'estat | cat |
dc.subject.classification | Treballs de fi de grau | cat |
dc.subject.other | Neutron stars | eng |
dc.subject.other | Equations of state | eng |
dc.subject.other | Bachelor's theses | eng |
dc.title | Equation of state for neutron star calculations | eng |
dc.type | info:eu-repo/semantics/bachelorThesis | ca |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | ca |
Appears in Collections: | Treballs Finals de Grau (TFG) - Física |
Files in This Item:
File | Description | Size | Format | |
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VIVES MORELL RAQUEL_474039.pdf | 297.95 kB | Adobe PDF | View/Open |
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