Natural inflation with 2 light quarks

dc.contributor.advisor	Notari, Alessio
dc.contributor.author	Garí Galíndez, Jon
dc.date.accessioned	2019-10-02T13:03:50Z
dc.date.available	2019-10-02T13:03:50Z
dc.date.issued	2019-06
dc.description	Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2019, Tutor: Alessio Notari	ca
dc.description.abstract	Natural 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 quark	ca
dc.format.extent	4 p.
dc.format.mimetype	application/pdf
dc.identifier.uri	https://hdl.handle.net/2445/141523
dc.language.iso	eng	ca
dc.rights	cc-by-nc-nd (c) Garí, 2019
dc.rights.accessRights	info:eu-repo/semantics/openAccess	ca
dc.rights.uri	http://creativecommons.org/licenses/by-nc-nd/3.0/es/	*
dc.source	Treballs Finals de Grau (TFG) - Física
dc.subject.classification	Cosmologia	cat
dc.subject.classification	Quarks	cat
dc.subject.classification	Treballs de fi de grau	cat
dc.subject.other	Cosmology	eng
dc.subject.other	Quarks	eng
dc.subject.other	Bachelor's theses	eng
dc.title	Natural inflation with 2 light quarks	eng
dc.type	info:eu-repo/semantics/bachelorThesis	ca

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