Are SP91 and COBE Inconsistent with Cold Dark Matter?

We present results on the consistency of standard cold dark matter (CDM) models with both the COBE normalization and the data from the 4th channel of the 9-point South Pole scan. We find that CDM models are consistent with both experiments, a conclusion which is at odds with some other analyses. Thi...

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Main Authors: Bunn, F, White, M, Srednicki, M, Scott, D
Language:English
Published: 1994
Subjects:
Online Access:http://cds.cern.ch/record/542933
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spelling ftcern:oai:cds.cern.ch:542933 2023-05-15T18:22:05+02:00 Are SP91 and COBE Inconsistent with Cold Dark Matter? Bunn, F White, M Srednicki, M Scott, D 1994 http://cds.cern.ch/record/542933 eng eng http://cds.cern.ch/record/542933 astro-ph/9308021 oai:cds.cern.ch:542933 Astrophysics and Astronomy 1994 ftcern 2018-07-28T05:22:47Z We present results on the consistency of standard cold dark matter (CDM) models with both the COBE normalization and the data from the 4th channel of the 9-point South Pole scan. We find that CDM models are consistent with both experiments, a conclusion which is at odds with some other analyses. This is partly due to our careful treatment of the temperature autocorrelation function, but also derives from a realization that the statistical conclusions depend strongly on assumptions about the prior distribution for the normalization $Q$. 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
Bunn, F
White, M
Srednicki, M
Scott, D
Are SP91 and COBE Inconsistent with Cold Dark Matter?
topic_facet Astrophysics and Astronomy
description We present results on the consistency of standard cold dark matter (CDM) models with both the COBE normalization and the data from the 4th channel of the 9-point South Pole scan. We find that CDM models are consistent with both experiments, a conclusion which is at odds with some other analyses. This is partly due to our careful treatment of the temperature autocorrelation function, but also derives from a realization that the statistical conclusions depend strongly on assumptions about the prior distribution for the normalization $Q$.
author Bunn, F
White, M
Srednicki, M
Scott, D
author_facet Bunn, F
White, M
Srednicki, M
Scott, D
author_sort Bunn, F
title Are SP91 and COBE Inconsistent with Cold Dark Matter?
title_short Are SP91 and COBE Inconsistent with Cold Dark Matter?
title_full Are SP91 and COBE Inconsistent with Cold Dark Matter?
title_fullStr Are SP91 and COBE Inconsistent with Cold Dark Matter?
title_full_unstemmed Are SP91 and COBE Inconsistent with Cold Dark Matter?
title_sort are sp91 and cobe inconsistent with cold dark matter?
publishDate 1994
url http://cds.cern.ch/record/542933
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation http://cds.cern.ch/record/542933
astro-ph/9308021
oai:cds.cern.ch:542933
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