Galactic anisotropy of Ultra-High Energy Cosmic Rays produced by CDM-related mechanisms

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dc.creatorDubovsky, S. L.
dc.creatorTinyakov, P. G.
dc.date1998-10-19
dc.date.accessioned2026-07-07T04:05:28Z
dc.date.available2026-07-07T04:05:28Z
dc.descriptionWe briefly review current theoretical and experimental status of Ultra-High Energy Cosmic Rays. We show that ``top-down'' mechanisms of UHE CR which involve heavy relic particle-like objects predict Galactic anisotropy of highest energy cosmic rays at the level of minimum $\sim 20%$. This anisotropy is large enough to be either observed or ruled out in the next generation of experiments.
dc.description10 pages; talk presented at the 10th International Seminar ``Quarks-98'', Suzdal, Russia, May 18-24, 1998; to appear in the Proceedings
dc.identifierhttps://arxiv.org/abs/hep-ph/9810401
dc.identifierhttp://arxiv.org/abs/hep-ph/9810401
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/48418
dc.subjectHigh Energy Physics - Phenomenology
dc.titleGalactic anisotropy of Ultra-High Energy Cosmic Rays produced by CDM-related mechanisms
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