PIRSA:10040090

Video URL

https://pirsa.org/10040090

Fingerprints of structure formation in the microwave background

Holder, G. (2010). Fingerprints of structure formation in the microwave background. Perimeter Institute for Theoretical Physics. https://pirsa.org/10040090

Holder, Gilbert. Fingerprints of structure formation in the microwave background. Perimeter Institute for Theoretical Physics, Apr. 28, 2010, https://pirsa.org/10040090 

          @misc{ scivideos_PIRSA:10040090,
            doi = {10.48660/10040090},
            url = {https://pirsa.org/10040090},
            author = {Holder, Gilbert},
            keywords = {Cosmology},
            language = {en},
            title = {Fingerprints of structure formation in the microwave background},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2010},
            month = {apr},
            note = {PIRSA:10040090 see, \url{https://scivideos.org/pirsa/10040090}}
          }

Gilbert Holder University of Illinois Urbana-Champaign

Talk numberPIRSA:10040090
DOI10.48660/10040090
Source RepositoryPIRSA
Collection
Talk Type Conference
Subject

Abstract

Non-linear structures in the universe leave characteristic imprints in the cosmic microwave background. These include Compton scattering (Sunyaev-Zeldovich effects) and gravitational lensing. The South Pole Telescope now has a catalog of massive galaxy clusters that were discovered this way, along with a measure of the background fluctuations generated by smaller clusters, that can be used to chart the growth of structure in the universe.