Understanding the Cosmic Microwave Background and its relevance in Cosmology

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dc.contributor.advisorManrique Oliva, Alberto
dc.contributor.authorFernández Bonet, David
dc.date.accessioned2020-10-14T15:25:15Z
dc.date.available2020-10-14T15:25:15Z
dc.date.issued2020-06
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Alberto Manriqueca
dc.description.abstractThe Cosmic Microwave Background (hereafter CMB) allows the accurate determination of cosmological parameters upon a careful study of its temperature anisotropies. In this work, physical phenomena that give rise to such anisotropies are discussed, along with an exhaustive analysis on the impact of baryon and dark matter density over the power spectrum's shape by using an online simulator. Finally, a sky map, illustrating the spatial distribution of temperature anisotropies, is generated.ca
dc.format.extent5 p.
dc.format.mimetypeapplication/pdf
dc.identifier.urihttps://hdl.handle.net/2445/171205
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Fernández Bonet, 2020
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.sourceTreballs Finals de Grau (TFG) - Física
dc.subject.classificationRadiació còsmica de fonscat
dc.subject.classificationAnisotropiacat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherCosmic microwave backgroundeng
dc.subject.otherAnisotropyeng
dc.subject.otherBachelor's theseseng
dc.titleUnderstanding the Cosmic Microwave Background and its relevance in Cosmologyeng
dc.typeinfo:eu-repo/semantics/bachelorThesisca

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