1. Dipòsit Digital de la Universitat de Barcelona
  2. Treballs de l'alumnat
  3. Treballs Finals de Grau (TFG) - Física
Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/141523
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dc.contributor.advisorNotari, Alessio-
dc.contributor.authorGarí Galíndez, Jon-
dc.date.accessioned2019-10-02T13:03:50Z-
dc.date.available2019-10-02T13:03:50Z-
dc.date.issued2019-06-
dc.identifier.urihttp://hdl.handle.net/2445/141523-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2019, Tutor: Alessio Notarica
dc.description.abstractNatural inflation is one of the most interesting models of inflation, it is generally studied for 1 light quark and is a model that fits with the experimental observations of the CMB within 2 sigma error. We will analyse the behaviour of a model of natural inflation with 2 light quarks and compare with observations. We will find that this model starts to be acceptable within 2 sigma when 𝑚𝑢𝑚𝑑⁄>4, otherwise the results are worse than the natural inflation with only 1 light quarkca
dc.format.extent4 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Garí, 2019-
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.sourceTreballs Finals de Grau (TFG) - Física-
dc.subject.classificationCosmologiacat
dc.subject.classificationQuarkscat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherCosmologyeng
dc.subject.otherQuarkseng
dc.subject.otherBachelor's theseseng
dc.titleNatural inflation with 2 light quarkseng
dc.typeinfo:eu-repo/semantics/bachelorThesisca
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
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