Implications of MAX for CDM

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dc.creatorSrednicki, Mark
dc.creatorWhite, Martin
dc.creatorScott, Douglas
dc.creatorBunn, Emory T.
dc.date1993-09-01
dc.date.accessioned2026-07-07T12:01:00Z
dc.date.available2026-07-07T12:01:00Z
dc.descriptionWe analyze the Gamma Ursae Minoris (GUM) and Mu Pegasii (MuP) scans of the Millimeter-wave Anisotropy eXperiment in the context of cold dark matter (CDM) models of structure formation, paying particular attention to the two-dimensional nature of the GUM scan. If all of the structure in the (foreground subtracted) data is attributed to cosmic microwave background anisotropy, then there is a detection in each scan. For a standard CDM model, the amplitudes of the signals are individually compatible with the COsmic Background Explorer measurement, but marginally inconsistent with each other.
dc.description10 pages in Plain TeX + 3 PS figures, CfPA-93-TH-27
dc.identifierhttps://arxiv.org/abs/astro-ph/9309006
dc.identifierhttp://arxiv.org/abs/astro-ph/9309006
dc.identifierPhys.Rev.Lett.71:3747,1993
dc.identifierdoi:10.1103/PhysRevLett.71.3747
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/206967
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleImplications of MAX for CDM
dc.typetext

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