Signatures of Cosmic Structure Formation in the Microwave Background ...

On small scales the cosmic microwave background (CMB) is perturbed by large scale structure in the universe, primarily through Compton scattering and gravitational lensing. The current generation of CMB experiments is measuring these signals, allowing new measurements of the build-up of cosmic struc...

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Format: Article in Journal/Newspaper
Language:English
Published: Perimeter Institute 2011
Subjects:
Online Access:https://dx.doi.org/10.48660/11030069
https://pirsa.org/11030069
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spelling ftdatacite:10.48660/11030069 2024-03-31T07:55:23+00:00 Signatures of Cosmic Structure Formation in the Microwave Background ... 2011 video/mp4 https://dx.doi.org/10.48660/11030069 https://pirsa.org/11030069 en eng Perimeter Institute Particle Physics Audiovisual Video Recording article MediaObject 2011 ftdatacite https://doi.org/10.48660/11030069 2024-03-04T13:30:01Z On small scales the cosmic microwave background (CMB) is perturbed by large scale structure in the universe, primarily through Compton scattering and gravitational lensing. The current generation of CMB experiments is measuring these signals, allowing new measurements of the build-up of cosmic structure. I will discuss two such measurements being made with the South Pole Telescope: 1) through Compton scattering (the Sunyaev-Zeldovich effect) we have compiled a large catalog of very massive galaxy clusters extending to z>1, allowing a measure of the growth of structure from z=1 to today; 2) we are currently measuring the gravitational lensing of the CMB, providing an accurate measure of the integrated structure between z=0 and z=1100. Both of these are powerful new tests of our cosmological understanding. ... Article in Journal/Newspaper South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language English
topic Particle Physics
spellingShingle Particle Physics
Signatures of Cosmic Structure Formation in the Microwave Background ...
topic_facet Particle Physics
description On small scales the cosmic microwave background (CMB) is perturbed by large scale structure in the universe, primarily through Compton scattering and gravitational lensing. The current generation of CMB experiments is measuring these signals, allowing new measurements of the build-up of cosmic structure. I will discuss two such measurements being made with the South Pole Telescope: 1) through Compton scattering (the Sunyaev-Zeldovich effect) we have compiled a large catalog of very massive galaxy clusters extending to z>1, allowing a measure of the growth of structure from z=1 to today; 2) we are currently measuring the gravitational lensing of the CMB, providing an accurate measure of the integrated structure between z=0 and z=1100. Both of these are powerful new tests of our cosmological understanding. ...
format Article in Journal/Newspaper
title Signatures of Cosmic Structure Formation in the Microwave Background ...
title_short Signatures of Cosmic Structure Formation in the Microwave Background ...
title_full Signatures of Cosmic Structure Formation in the Microwave Background ...
title_fullStr Signatures of Cosmic Structure Formation in the Microwave Background ...
title_full_unstemmed Signatures of Cosmic Structure Formation in the Microwave Background ...
title_sort signatures of cosmic structure formation in the microwave background ...
publisher Perimeter Institute
publishDate 2011
url https://dx.doi.org/10.48660/11030069
https://pirsa.org/11030069
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_doi https://doi.org/10.48660/11030069
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