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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Online Access: | https://dx.doi.org/10.48660/11030069 https://pirsa.org/11030069 |
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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 |
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Open Polar |
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DataCite Metadata Store (German National Library of Science and Technology) |
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ftdatacite |
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English |
topic |
Particle Physics |
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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 |
_version_ |
1795037211845984256 |