Observational Constraints on Open Inflation Models

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dc.creatorWhite, Martin
dc.creatorSilk, Joe
dc.date1996-08-27
dc.date1997-03-28
dc.date.accessioned2026-07-07T12:01:04Z
dc.date.available2026-07-07T12:01:04Z
dc.descriptionWe discuss observational constraints on models of open inflation. Current data from large-scale structure and the cosmic microwave background prefer models with blue spectra and/or Omega_0 >= 0.3--0.5. Models with minimal anisotropy at large angles are strongly preferred.
dc.description4 pages, RevTeX, with 2 postscript figures included. Second Figure corrected
dc.identifierhttps://arxiv.org/abs/astro-ph/9608177
dc.identifierhttp://arxiv.org/abs/astro-ph/9608177
dc.identifierPhys.Rev.Lett.77:4704-4707,1996; Erratum-ibid.78:3799,1997
dc.identifierdoi:10.1103/PhysRevLett.77.4704
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/206984
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleObservational Constraints on Open Inflation Models
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