Video URL

https://pirsa.org/16120032

Breaking inflation with inhomogeneous initial conditions

Clough, K. (2016). Breaking inflation with inhomogeneous initial conditions. Perimeter Institute for Theoretical Physics. https://pirsa.org/16120032

Clough, Katy. Breaking inflation with inhomogeneous initial conditions. Perimeter Institute for Theoretical Physics, Dec. 13, 2016, https://pirsa.org/16120032 

          @misc{ scivideos_PIRSA:16120032,
            doi = {10.48660/16120032},
            url = {https://pirsa.org/16120032},
            author = {Clough, Katy},
            keywords = {Cosmology},
            language = {en},
            title = {Breaking inflation with inhomogeneous initial conditions},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2016},
            month = {dec},
            note = {PIRSA:16120032 see, \url{https://scivideos.org/pirsa/16120032}}
          }

Katy Clough University of Göttingen

DOI 10.48660/16120032
Source Repository PIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Inflation is proposed as a means of explaining why the Universe is currently so homogeneous on larger scales, solving both the horizon and flatness problems in early universe cosmology. However, if inflation itself requires homogeneous conditions to get started, then inflation is not a solution to the horizon problem. Most work up until now has focussed on a dynamical systems approach to classifying the stability of inflationary models, but recently Numerical Relativity (NR) has been used to simulate the actual evolution of the inflaton field, leading to new insights. I will describe a recent work (https://arxiv.org/abs/1608.04408) in which we used NR to consider the robustness of generic small and large field inflationary models to initial inhomogeneities in the inflaton field and the extrinsic curvature of the metric.