The Impact of COBE on Inflation, Dark Matter, and Structure Formation: a Brief Review

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dc.creatorKrauss, Lawrence M.
dc.date1993-06-08
dc.date.accessioned2026-07-07T03:56:07Z
dc.date.available2026-07-07T03:56:07Z
dc.descriptionThe COBE results, to be followed in the near future by other Cosmic Microwave Background measurements, are providing us with a new fundamental tool to probe the formation of large scale structure in the Universe, and in so doing to constrain our models of the early universe and the nature of dark matter. I describe briefly here how to interpret the COBE results data with these in mind, and conclude with a discussion of implications for the future.
dc.descriptionBased upon lectures at the 5th International Workshop on Neutrino Telescopes, Venice, and the Rencontres de Physique de la Vallee d'Aoste, La Thuile, March 1993, 16 pages plus one figure (not included); binhex'ed macword
dc.identifierhttps://arxiv.org/abs/hep-ph/9306247
dc.identifierhttp://arxiv.org/abs/hep-ph/9306247
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44826
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleThe Impact of COBE on Inflation, Dark Matter, and Structure Formation: a Brief Review
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