Measuring Cosmological Parameters with Cosmic Microwave Background Experiments

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dc.creatorBond, J. R.
dc.creatorCrittenden, Robert
dc.creatorDavis, Richard L.
dc.creatorEfstathiou, George
dc.creatorSteinhardt, Paul J.
dc.date1993-09-28
dc.date1993-10-06
dc.date.accessioned2026-07-07T10:34:48Z
dc.date.available2026-07-07T10:34:48Z
dc.descriptionThe cosmic microwave background anisotropy is sensitive to the slope and amplitude of primordial energy density and gravitational wave fluctuations, the baryon density, the Hubble constant, the cosmological constant, the ionization history, {\it etc.} In this Letter, we examine the degree to which these factors can be separately resolved from combined small- and large-angular scale anisotropy observations. We isolate directions of degeneracy in this cosmic parameter space, but note that other cosmic observations can break the degeneracy. (Correction to Eq. 4)
dc.description10 pages, Penn Preprint
dc.identifierhttps://arxiv.org/abs/astro-ph/9309041
dc.identifierhttp://arxiv.org/abs/astro-ph/9309041
dc.identifierPhys.Rev.Lett.72:13-16,1994
dc.identifierdoi:10.1103/PhysRevLett.72.13
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179562
dc.subjectAstrophysics
dc.titleMeasuring Cosmological Parameters with Cosmic Microwave Background Experiments
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