Evidence for Compact Dark Matter in Galactic Halos

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dc.creatorAbbas, S.
dc.creatorAbbas, A.
dc.creatorMohanty, S.
dc.date1999-10-11
dc.date1999-11-21
dc.date.accessioned2026-07-07T02:33:46Z
dc.date.available2026-07-07T02:33:46Z
dc.descriptionClumped dark matter arises naturally within the framwork of generic cosmological dark matter models. Invoking the existence of dark matter clumps can also solve may unexplained mysteries in astrophysics and geology or geophysics, eg. the galactic gamma-ray halo and the periodic terrestrial flood basalt volcanic episodes. Clumped dark matter is dynamically stable to friction and will not heat the disk. Such clumps may have already been discovered in the form of dwarf spheroidals, and further searches are encouraged by the results of this paper.
dc.descriptionRevised Version, includes new relevant references, Latex File, 16 pages, no figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9910187
dc.identifierhttp://arxiv.org/abs/astro-ph/9910187
dc.identifierIndian J.Phys. B74 (2000) 179
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14980
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectGeophysics
dc.titleEvidence for Compact Dark Matter in Galactic Halos
dc.typetext

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