Show simple item record

dc.contributor.authorChristopherson, Adam J.
dc.date.accessioned2011-07-12T14:32:50Z
dc.date.available2011-07-12T14:32:50Z
dc.date.issued2011
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/1308
dc.descriptionPhDen_US
dc.description.abstractCosmological perturbation theory is crucial for our understanding of the universe. The linear theory has been well understood for some time, however developing and applying the theory beyond linear order is currently at the forefront of research in theoretical cosmology. This thesis studies the applications of perturbation theory to cosmology and, speci cally, to the early universe. Starting with some background material introducing the well-tested `standard model' of cosmology, we move on to develop the formalism for perturbation theory up to second order giving evolution equations for all types of scalar, vector and tensor perturbations, both in gauge dependent and gauge invariant form. We then move on to the main result of the thesis, showing that, at second order in perturbation theory, vorticity is sourced by a coupling term quadratic in energy density and entropy perturbations. This source term implies a qualitative di erence to linear order. Thus, while at linear order vorticity decays with the expansion of the universe, the same is not true at higher orders. This will have important implications on future measurements of the polarisation of the Cosmic Microwave Background, and could give rise to the generation of a primordial seed magnetic eld. Having derived this qualitative result, we then estimate the scale dependence and magnitude of the vorticity power spectrum, nding, for simple power law inputs a small, blue spectrum. The nal part of this thesis concerns higher order perturbation theory, deriving, for the rst time, the metric tensor, gauge transformation rules and governing equations for fully general third order perturbations. We close with a discussion of natural extensions to this work and other possible ideas for o -shooting projects in this continually growing eld.en_US
dc.language.isoenen_US
dc.subjectAstronomyen_US
dc.titleApplications of cosmological perturbation theoryen_US
dc.typeThesisen_US
dc.rights.holderThe 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


Files in this item

Thumbnail

This item appears in the following Collection(s)

  • Theses [2752]
    Theses Awarded by Queen Mary University of London

Show simple item record