PIRSA:15080017

CMB Anomalies and Non-Gaussianity

Shandera, S. (2015). CMB Anomalies and Non-Gaussianity. Perimeter Institute. https://pirsa.org/15080017

Shandera, Sarah. CMB Anomalies and Non-Gaussianity. Perimeter Institute, Aug. 10, 2015, https://pirsa.org/15080017 

          @misc{ pirsa_PIRSA:15080017,
            doi = {10.48660/15080017},
            url = {https://pirsa.org/15080017},
            author = {Shandera, Sarah},
            keywords = {Cosmology, Other},
            language = {en},
            title = {CMB Anomalies and Non-Gaussianity},
            publisher = {Perimeter Institute},
            year = {2015},
            month = {aug},
            note = {PIRSA:15080017 see, \url{https://pirsa.org}}
          }

Sarah Shandera

Pennsylvania State University

Talk number
PIRSA:15080017
Collection
Talk Type
Subject
Abstract
When the primordial fluctuations are non-Gaussian and inflation lasts longer than the minimum number of e-folds, the likelihood that we observe mild deviations from isotropy increases. I will present a single framework that encompasses many of the most promising scenarios for generating a hemispherical power asymmetry. This framework allows a comparison of the observational evidence for various models, including some with a natural connection between large scale power suppression and power asymmetry.