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Why Do We Need Non-Baryonic Dark Matter?

1996/05/14 by Keith A. Olive, Olive, Keith A.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Quantum Mechanics and Applications #Radioactive Decay and Measurement Techniques #Relativity and Gravitational Theory #astro-ph #hep-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/9605068

22 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

arxiv created 1996/05/14 · openalex publication_date 1996/05/14 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Observational evidence along with theoretical arguments which call for non-baryonic dark matter are reviewed. A brief summary of the dark matter session is included.

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