1993/01/01 by Lawrence M. Krauss, Krauss, Lawrence M.
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics (astro-ph) #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #Geophysics and Gravity Measurements #High Energy Physics - Phenomenology (hep-ph) #astro-ph #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/9306247
Based 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
openalex publication_date 1993/01/01 · arxiv created 1993/06/08 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The 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.