PIRSA:09050051

Video URL

https://pirsa.org/09050051

Bispectrum signatures of modifications to the inflationary vacuum

van der Schaar, J.P. (2009). Bispectrum signatures of modifications to the inflationary vacuum. Perimeter Institute for Theoretical Physics. https://pirsa.org/09050051

van der Schaar, Jan Pieter. Bispectrum signatures of modifications to the inflationary vacuum. Perimeter Institute for Theoretical Physics, May. 20, 2009, https://pirsa.org/09050051 

          @misc{ scivideos_PIRSA:09050051,
            doi = {10.48660/09050051},
            url = {https://pirsa.org/09050051},
            author = {van der Schaar, Jan Pieter},
            keywords = {Cosmology},
            language = {en},
            title = {Bispectrum signatures of modifications to the inflationary vacuum},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2009},
            month = {may},
            note = {PIRSA:09050051 see, \url{https://scivideos.org/pirsa/09050051}}
          }

Jan Pieter van der Schaar Universiteit van Amsterdam

Talk numberPIRSA:09050051
DOI10.48660/09050051
Source RepositoryPIRSA
Collection
Talk Type Conference
Subject

Abstract

Modifications of the initial-state of the inflaton field can induce a departure from Gaussianity and leave a testable imprint on the higher order correlations of the CMB and large scale structures in the Universe. I will discuss general vacuum state modifications in the case of a canonical single-field action, after adding a dimension 8 higher order derivative term, and DBI models of inflation. Observed bounds on local and equilateral non-Gaussianities, even though they correspond to template shapes that are far from optimal, can lead to constraints that are already competing to those derived from the power spectrum alone, due to enhancement effects. We emphasize that the construction and application of especially adapted templates could lead to significant improvements in the CMB bispectrum constraints on modified initial states.