Density Fluctuations in the Galactic Halo and Experimental Searches for Dark Matter

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dc.creatorWasserman, Ira
dc.date1996-08-02
dc.date.accessioned2026-07-07T02:21:42Z
dc.date.available2026-07-07T02:21:42Z
dc.descriptionClumping of elementary dark matter in the Galaxy halo may be inevitable. If so, the nondetection of certain dark matter candidates could simply mean that the local halo density is low. Conversely, indirect detection of annihilation products could be facilitated, perhaps to an embarrassing degree.
dc.description3 pages; Second Sakharov Conference on Physics, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/9608012
dc.identifierhttp://arxiv.org/abs/astro-ph/9608012
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10601
dc.subjectAstrophysics
dc.titleDensity Fluctuations in the Galactic Halo and Experimental Searches for Dark Matter
dc.typetext

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