Spectator fields and their imprints on the Cosmic Microwave Background

Wang, Lingfei (2016) Spectator fields and their imprints on the Cosmic Microwave Background. PhD thesis, UNSPECIFIED.

[img]
Preview
PDF (2016wangphd)
2016wangphd.pdf - Published Version
Available under License Creative Commons Attribution-NoDerivs.

Download (8MB)

Abstract

When a subdominant light scalar field ends slow roll during inflation, but well after the Hubble exit of the pivot scales, it may determine the cosmological perturbations. This thesis investigates how such a scalar field, the spectator, may leave its impact on the Cosmic Microwave Background (CMB) radiation and be consequently constrained. We first introduce the observables of the CMB, namely the power spectrum Pζ , spectral index ns and its running dns/d ln k, the non-Gaussianities fNL, gNL and τNL, and the lack of isocurvature and polarization modes. Based on these studies, we derive the cosmological predictions for the spectator scenario, revealing its consistency with the CMB for inflection point potentials, hyperbolic tangent potentials, and those with a sudden phase transition. In the end, we utilize the spectator scenario to explain the CMB power asymmetry, with a brief tachyonic fast-roll phase.

Item Type: Thesis (PhD)
Departments: Faculty of Science and Technology > Physics
ID Code: 83591
Deposited By: ep_importer_pure
Deposited On: 14 Dec 2016 10:02
Refereed?: No
Published?: Published
Last Modified: 14 Oct 2019 10:06
URI: https://eprints.lancs.ac.uk/id/eprint/83591

Actions (login required)

View Item View Item