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dc.contributor.authorCARRILHO, PEDROen_US
dc.date.accessioned2019-04-12T15:09:32Z
dc.date.issued2019-03-07en_US
dc.identifier.urihttps://qmro.qmul.ac.uk/xmlui/handle/123456789/56860
dc.descriptionPhD thesisen_US
dc.description.abstractIn this thesis, we discuss several instances in which non-linear behaviour affects cosmological evolution in the early Universe. We begin by reviewing the standard cosmological model and the tools used to understand it theoretically and to compute its observational consequences. This includes a detailed exposition of cosmological perturbation theory and the theory of inflation. We then describe the results in this thesis, starting with the non-linear evolution of the curvature perturbation in the presence of vector and tensor fluctuations, in which we identify the version of that variable that is conserved in the most general situation. Next, we use second order perturbation theory to describe the most general initial conditions for the evolution of scalar perturbations at second order in the standard cosmological model. We compute approximate solutions valid in the initial stages of the evolution, which can be used to initialize second order Boltzmann codes, and to compute many observables taking isocurvature modes into account. We then move on to the study of the inflationary Uiniverse. We start by analysing a new way to compute the consequences of a sudden transition in the evolution of a scalar during inflation. We use the formalism of quantum quenches to compute the effect of those transitions on the spectral index of perturbations. Finally, we detail the results of the exploration of a multi- field model of inflation with a non-minimal coupling to gravity. We study popular attractor models in this regime in both the metric and the Palatini formulations of gravity and fi nd all results for both the power spectrum and bispectrum of fluctuations to closely resemble those of the single- field case. In all systems under study we discuss the effects of non-linear dynamics and their importance for the resolution of problems in cosmology.en_US
dc.description.sponsorshipQueen Mary Principal's Research Studentshipen_US
dc.description.sponsorshipBolsa de Excel^encia Acad emica of the Funda c~ao Eug enio de Almeida from 2014 to 2017en_US
dc.description.sponsorshipFunda c~ao para a Ci^encia e Tecnologia (FCT) grant SFRH/BD/118740/2016 from 2017 to 2018en_US
dc.language.isoenen_US
dc.publisherQueen Mary University of London
dc.rightsThe copyright of this thesis rests with the author and no quotation from it or information derived from it may be published without the prior written consent of the author
dc.subjectSchool of Physics and Astronomyen_US
dc.subjectAstronomy Uniten_US
dc.subjectphysics of the early universeen_US
dc.titleNon-linear effects in early Universe cosmologyen_US
pubs.notesNot knownen_US
rioxxterms.funderDefault funderen_US
rioxxterms.identifier.projectDefault projecten_US


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    Theses Awarded by Queen Mary University of London

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