Video URL

https://pirsa.org/07100004

Constraints on scale dependent non-Gaussianity

Shandera, S. (2007). Constraints on scale dependent non-Gaussianity. Perimeter Institute for Theoretical Physics. https://pirsa.org/07100004

Shandera, Sarah. Constraints on scale dependent non-Gaussianity. Perimeter Institute for Theoretical Physics, Oct. 30, 2007, https://pirsa.org/07100004 

          @misc{ scivideos_PIRSA:07100004,
            doi = {10.48660/07100004},
            url = {https://pirsa.org/07100004},
            author = {Shandera, Sarah},
            keywords = {Cosmology},
            language = {en},
            title = {Constraints on scale dependent non-Gaussianity},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2007},
            month = {oct},
            note = {PIRSA:07100004 see, \url{https://scivideos.org/index.php/pirsa/07100004}}
          }

Sarah Shandera Pennsylvania State University

DOI 10.48660/07100004
Source Repository PIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

The detection of primordial non-Gaussianity could provide a powerful means to rule out various inflationary scenarios. Although scale-invariant non-Gaussianity is currently best constrained by the Cosmic Microwave Background, single-field inflation models with changing sound speed can have strongly scale dependent non-Gaussianity. I will discuss the theoretical motivation for such models and present work on the likely ability of current and future large scale structure measurements to constrain them.