1996/01/31 by V. Berezinsky, A. Bottino, G. Mignola
Physics and Astronomy · #Astrophysics #Axion #Baryon #Baryonic dark matter #Cold dark matter #Context (archaeology) #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark matter #Hot dark matter #Light dark matter #Mixed dark matter #Particle physics #Particle physics theoretical and experimental studies #Physics #Scalar field dark matter #Warm dark matter #astro-ph
paper · pdf · doi:10.1016/0920-5632(96)00199-5
published as Nucl.Phys.Proc.Suppl. 48 (1996) 22-33 · Latex, 12 pages, espcrc2.sty, 6 figures included, appended as a uuencoded compressed tarred file. Invited talk at the TAUP95 workshop, presented by V. Berezinsky
arxiv created 1996/01/31 · openalex publication_date 1996/05/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The best particle candidates for non--baryonic cold dark matter are reviewed, namely, neutralino, axion, axino and Majoron. These particles are considered in the context of cosmological models with the restrictions given by the observed mass spectrum of large scale structures, data on clusters of galaxies, age of the Universe etc.