Are SP91 and COBE Inconsistent with Cold Dark Matter?

Simple item page
dc.creatorBunn, E.
dc.creatorWhite, M.
dc.creatorSrednicki, M.
dc.creatorScott, D.
dc.date1993-08-17
dc.date1993-08-26
dc.date.accessioned2026-07-07T12:00:59Z
dc.date.available2026-07-07T12:00:59Z
dc.descriptionWe 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 $Q$.
dc.description8 pages in Plain TeX plus 2 PS figures; revisions consist of a correction to the method of offset and gradient subtraction, changing the numerical results by about 10\%; conclusions unchanged; CfPA-93-TH-20
dc.identifierhttps://arxiv.org/abs/astro-ph/9308021
dc.identifierhttp://arxiv.org/abs/astro-ph/9308021
dc.identifierAstrophys.J.429:1-3,1994
dc.identifierdoi:10.1086/174296
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/206966
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleAre SP91 and COBE Inconsistent with Cold Dark Matter?
dc.typetext

Files

Collections

arXiv