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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4878
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dc.contributor.authorPadmanabhan, T.-
dc.contributor.authorSethi, S.K.-
dc.date.accessioned2012-07-11T09:48:04Z-
dc.date.available2012-07-11T09:48:04Z-
dc.date.issued2001-07-
dc.identifier.citationThe Astrophysical Journal, 2001, Vol.555, p125en
dc.identifier.issn0004-637X-
dc.identifier.issn1538-4357(Online)-
dc.identifier.urihttp://hdl.handle.net/2289/4878-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractWe analyze the BOOMERANG and MAXIMA results in the context of simplest inflationary universes: ΩTotal=1, ns~=1. We attempt to constrain three other parameters-h, ΩB, and Ωm-from these observations. We show that (1) the data are consistent with the values of Ωm and h inferred from other observations and (2) the value of ΩBh2 is too high to be compatible with big bang nucleosynthesis observations at the 2 σ level for ns=1. We also include two cosmic background imager (CBI) band powers in our analysis. However, the inclusion of CBI band powers doesn't affect our conclusions.en
dc.language.isoenen
dc.publisherUniversity of Chicago Pressen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001ApJ...555..125Pen
dc.relation.urihttp://arxiv.org/abs/10.1086/321469en
dc.relation.urihttp://arxiv.org/abs/astro-ph/0010309en
dc.rights2001 University of Chicago Pressen
dc.subjectCosmologyen
dc.subjectCosmic Microwave Backgrounden
dc.subjectCosmology: Observationsen
dc.subjectCosmology: Theoryen
dc.titleConstraints on ΩB, Ωm, and h from MAXIMA and BOOMERANGen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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