Reionization and Cosmic Microwave Anisotropies

The effects of reionization, occurring after standard recombination in cold dark matter-dominated models, on CMB anisotropies are investigated. Late-time reionization reduces the CMB anisotropies, in particular, on degree scales. It is found that constraints on cold dark matter-dominated models from...

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Main Authors: Sugiyama, N, Silk, J, Vittorio, N
Language:English
Published: 1993
Subjects:
Online Access:http://cds.cern.ch/record/543455
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spelling ftcern:oai:cds.cern.ch:543455 2023-05-15T18:22:02+02:00 Reionization and Cosmic Microwave Anisotropies Sugiyama, N Silk, J Vittorio, N 1993-10-28 http://cds.cern.ch/record/543455 eng eng http://cds.cern.ch/record/543455 astro-ph/9310051 oai:cds.cern.ch:543455 Astrophysics and Astronomy 1993 ftcern 2018-07-28T05:23:15Z The effects of reionization, occurring after standard recombination in cold dark matter-dominated models, on CMB anisotropies are investigated. Late-time reionization reduces the CMB anisotropies, in particular, on degree scales. It is found that constraints on cold dark matter-dominated models from the highest frequency channel of the 9-point South Pole data are significantly relaxed for models which are consistent with Big Bang nucleosynthesis if reionization is assumed to have occurred by redshift $\sim 20.$ Other/Unknown Material South pole CERN Document Server (CDS) South Pole
institution Open Polar
collection CERN Document Server (CDS)
op_collection_id ftcern
language English
topic Astrophysics and Astronomy
spellingShingle Astrophysics and Astronomy
Sugiyama, N
Silk, J
Vittorio, N
Reionization and Cosmic Microwave Anisotropies
topic_facet Astrophysics and Astronomy
description The effects of reionization, occurring after standard recombination in cold dark matter-dominated models, on CMB anisotropies are investigated. Late-time reionization reduces the CMB anisotropies, in particular, on degree scales. It is found that constraints on cold dark matter-dominated models from the highest frequency channel of the 9-point South Pole data are significantly relaxed for models which are consistent with Big Bang nucleosynthesis if reionization is assumed to have occurred by redshift $\sim 20.$
author Sugiyama, N
Silk, J
Vittorio, N
author_facet Sugiyama, N
Silk, J
Vittorio, N
author_sort Sugiyama, N
title Reionization and Cosmic Microwave Anisotropies
title_short Reionization and Cosmic Microwave Anisotropies
title_full Reionization and Cosmic Microwave Anisotropies
title_fullStr Reionization and Cosmic Microwave Anisotropies
title_full_unstemmed Reionization and Cosmic Microwave Anisotropies
title_sort reionization and cosmic microwave anisotropies
publishDate 1993
url http://cds.cern.ch/record/543455
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation http://cds.cern.ch/record/543455
astro-ph/9310051
oai:cds.cern.ch:543455
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