Nuclear Matter at Finite Temperature

dc.contributor.advisor	Centelles Aixalà, Mario
dc.contributor.author	Bañuelos Sánchez, Arnau
dc.date.accessioned	2026-08-27T09:05:48Z
dc.date.available	2026-08-27T09:05:48Z
dc.date.issued	2026-06
dc.description	Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2026, Tutor: Mario Centelles
dc.description.abstract	In this work, we compute the equation of state of hot nuclear matter and study how thermodynamic quantities such as the entropy, free energy, and pressure evolve with temperature as functions of density. We also analyse the role of isospin asymmetry, showing how the relative neutron and proton content influences the stiffness of the equation of state and the saturation properties of the system. In addition, the free symmetry energy is evaluated as a measure of the isospin dependence of nuclear matter.
dc.format.extent	6 p.
dc.format.mimetype	application/pdf
dc.identifier.uri	https://hdl.handle.net/2445/231202
dc.language.iso	eng
dc.rights	cc-by-nc-nd (c) Bañuelos Sánchez, Arnau, 2026
dc.rights.accessRights	info:eu-repo/semantics/openAccess
dc.rights.uri	http://creativecommons.org/licenses/by-nc-nd/4.0/
dc.subject.classification	Equacions d'estat	cat
dc.subject.classification	Matèria nuclear	cat
dc.subject.classification	Treballs de fi de grau	cat
dc.subject.other	Equations of state	eng
dc.subject.other	Nuclear matter	eng
dc.subject.other	Bachelor's theses	eng
dc.title	Nuclear Matter at Finite Temperature
dc.type	info:eu-repo/semantics/bachelorThesis

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