Why Do We Need Non-Baryonic Dark Matter?

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dc.creatorOlive, Keith A.
dc.date1996-05-14
dc.date.accessioned2026-07-07T02:21:16Z
dc.date.available2026-07-07T02:21:16Z
dc.descriptionObservational evidence along with theoretical arguments which call for non-baryonic dark matter are reviewed. A brief summary of the dark matter session is included.
dc.description22 pages, latex, 7 ps figures, Combined Introductory and Summary talks delivered at the Dark Matter seesion at the XXXIst Recontres de Moriond, January 20-27, 1996
dc.identifierhttps://arxiv.org/abs/astro-ph/9605068
dc.identifierhttp://arxiv.org/abs/astro-ph/9605068
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10486
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleWhy Do We Need Non-Baryonic Dark Matter?
dc.typetext

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