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http://hdl.handle.net/2445/201118
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DC Field | Value | Language |
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dc.contributor.advisor | Centelles Aixalà, Mario | - |
dc.contributor.author | Hernández Toledo, Adrià | - |
dc.date.accessioned | 2023-07-25T08:34:44Z | - |
dc.date.available | 2023-07-25T08:34:44Z | - |
dc.date.issued | 2023-06 | - |
dc.identifier.uri | http://hdl.handle.net/2445/201118 | - |
dc.description | Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2023, Tutor: Mario Centelles Aixalà | ca |
dc.description.abstract | Symmetric nuclear matter, asymmetric nuclear matter and β-stable nuclear matter are discussed and modeled through a Lagrangian density of relativistic mean field (RMF) theory using a σ meson to describe the attractive interaction between nucleons, a ω meson to describe the repulsive interaction and a ρ meson to describe the asymmetry effects with the NL3 parametrization. | ca |
dc.format.extent | 5 p. | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | eng | ca |
dc.rights | cc-by-nc-nd (c) Hernández, 2023 | - |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ | * |
dc.source | Treballs Finals de Grau (TFG) - Física | - |
dc.subject.classification | Equació d'estat | cat |
dc.subject.classification | Estels de neutrons | cat |
dc.subject.classification | Treballs de fi de grau | cat |
dc.subject.other | Equation of state | eng |
dc.subject.other | Neutron stars | eng |
dc.subject.other | Bachelor's theses | eng |
dc.title | Calculation of the equation of state of neutron star matter | 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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HERNANDEZ TOLEDO ADRIA_7934176.pdf | 435.98 kB | Adobe PDF | View/Open |
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