Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/222435
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dc.contributor.advisorSolà Peracaula, Joan-
dc.contributor.authorBigorra Lorenzo, Víctor-Xavier-
dc.date.accessioned2025-07-22T07:03:41Z-
dc.date.available2025-07-22T07:03:41Z-
dc.date.issued2025-06-
dc.identifier.urihttps://hdl.handle.net/2445/222435-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2025, Tutor: Joan Solà Peracaulaca
dc.description.abstractWhile the vacuum energy and the cosmological constant are thought to be related, the exact connection is not well understood. In this work, we will consider the equation of state of the vacuum and other cosmic fluids potentially relevant for the description of the dark energy in the universe, in particular that of ‘phantom matter’, which is different from both dark matter and phantom dark energy. It is related to a form of false vacuum energy producing positive pressure, as ordinary matter (hence its name), but in contrast negative energy density. Some theoretical scenarios will be considered and also possible phenomenological implications.ca
dc.format.extent7 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Bigorra, 2025-
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.subject.classificationCosmologiacat
dc.subject.classificationEnergia fosca (Astronomia)cat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherCosmologyeng
dc.subject.otherDark energy (Astronomy)eng
dc.subject.otherBachelor's theseseng
dc.titlePhantom matter and vacuum energy: cosmological implicationseng
dc.typeinfo:eu-repo/semantics/bachelorThesisca
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
Appears in Collections:Treballs Finals de Grau (TFG) - Física

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