PIRSA:18010091

Video URL

https://pirsa.org/18010091

Gravitational lensing of the CMB: Self-consistency tests and other implications

Motloch, P. (2018). Gravitational lensing of the CMB: Self-consistency tests and other implications. Perimeter Institute for Theoretical Physics. https://pirsa.org/18010091

Motloch, Pavel. Gravitational lensing of the CMB: Self-consistency tests and other implications. Perimeter Institute for Theoretical Physics, Jan. 30, 2018, https://pirsa.org/18010091 

          @misc{ scivideos_PIRSA:18010091,
            doi = {10.48660/18010091},
            url = {https://pirsa.org/18010091},
            author = {Motloch, Pavel},
            keywords = {Cosmology},
            language = {en},
            title = {Gravitational lensing of the CMB: Self-consistency tests and other implications},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2018},
            month = {jan},
            note = {PIRSA:18010091 see, \url{https://scivideos.org/pirsa/18010091}}
          }

Pavel Motloch University of Chicago

Talk numberPIRSA:18010091
DOI10.48660/18010091
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Cosmic microwave background (CMB) experiments, which currently provide some of the most powerful cosmological data sets, will become much more constraining in the near future. While these measurements promise to teach us more about the nature of dark energy, inflation and neutrino physics, increased precision will require special attention dedicated to the data analysis. In this talk I will focus on the gravitational lensing of the CMB and some of its implications. By introducing a novel analysis technique, applying it to the Planck satellite data and commenting on improvements which will be possible with a CMB Stage 4 experiment, I will first show how we can utilize CMB gravitational lensing to probe self-consistency of the CMB data sets. Then I will overview how gravitational lensing induces non-Gaussian covariances between the CMB data and how these covariances affect constraints on the cosmological parameters.