Derivation of Friedman Equations

dc.contributor.advisorSalvador Solé, Eduard
dc.contributor.authorArnau Romeu, Joan
dc.date.accessioned2014-11-18T11:59:06Z
dc.date.available2014-11-18T11:59:06Z
dc.date.issued2014-06
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Any: 2014, Tutor: Eduard Salvador Soléca
dc.description.abstractIn this report we make a detailed derivation of Friedman Equations, which are the dy- namical equations of a homogeneous and isotropic universe. First, we derive them in the framework of the General Relativity keeping the relativistic expressions as a reference for the rest of the report. Then, using the Newtonian formalism and solving some fundamental problems, we reach some dy- namical equations for the universe and compare the results with the relativistic ones, focusing our attention on the meaning of the expressions and on the cosmological constant.ca
dc.format.extent5 p.
dc.format.mimetypeapplication/pdf
dc.identifier.urihttps://hdl.handle.net/2445/59759
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Salvador Solé, 2014
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.classificationCosmologia quànticacat
dc.subject.classificationEquacionscat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherQuantum cosmologyeng
dc.subject.otherEquationseng
dc.subject.otherBachelor's theseseng
dc.titleDerivation of Friedman Equationseng
dc.typeinfo:eu-repo/semantics/bachelorThesisca

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