Probing the Early Universe with the S-Z Effect

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dc.creatorJoy, Marshall
dc.creatorCarlstrom, John E.
dc.date2001-03-12
dc.date2001-03-13
dc.date.accessioned2026-07-07T01:57:56Z
dc.date.available2026-07-07T01:57:56Z
dc.descriptionThe cosmic microwave background radiation (CMBR) is providing important clues into the evolution of the early universe. In this Science Perspective, Joy and Carlstrom discuss one feature of the CMBR, the Sunyaev-Zel'dovich effect, which can be used to determine the abundance and evolution of clusters of galaxies, thereby constraining key cosmological parameters such as the matter density of the universe and its expansion rate.
dc.descriptionScience Perspective article. 3 pages, including 2 figures. Version 2 corrects a typographical error
dc.identifierhttps://arxiv.org/abs/astro-ph/0103177
dc.identifierhttp://arxiv.org/abs/astro-ph/0103177
dc.identifierScience, volume 291, pages 1715-1717, March 2, 2001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2582
dc.subjectAstrophysics
dc.titleProbing the Early Universe with the S-Z Effect
dc.typetext

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