Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/115062
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dc.contributor.advisorSolà Peracaula, Joan-
dc.contributor.authorPineda Romero., Àlvar-
dc.date.accessioned2017-09-06T17:06:14Z-
dc.date.available2017-09-06T17:06:14Z-
dc.date.issued2017-01-
dc.identifier.urihttp://hdl.handle.net/2445/115062-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2017, Tutor: Joan Solàcat
dc.description.abstractThe most common explanation for the dark energy corresponds to the standard [lambda]CDM model but it has some huge problems such as the Cosmological Constant Problem [1]. Thus, it is reasonable to search for alternative dark energy models. For this purpose, in this work we study the properties of a set of dynamical dark energy models different from the traditional scalar field approach (Quintessence and the like). Based on our results, and also on previous studies [2], we find that the [lambda]CDM hypothesis [lambda ]= const might not be the best description of the observational data.eng
dc.format.extent5 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengeng
dc.rightscc-by-nc-nd (c) Pineda, 2017-
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/-
dc.subject.classificationEnergia fosca (Astronomia)cat
dc.subject.classificationExpansió de l'universcat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherDark energy (Astronomy)eng
dc.subject.otherExpanding universeeng
dc.subject.otherBachelor's thesiseng
dc.titleModels of dynamical dark energy in the expanding Universeeng
dc.typeinfo:eu-repo/semantics/bachelorThesiseng
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesseng
Appears in Collections:Treballs Finals de Grau (TFG) - Física

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