Detectability of the Sgr Dwarf Leading Tidal Stream with Auger, EUSO or OWL

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dc.creatorGelmini, Graciela
dc.creatorGondolo, Paolo
dc.creatorSoldatenko, Adrian
dc.date2003-10-31
dc.date2004-06-23
dc.date.accessioned2026-07-07T11:31:30Z
dc.date.available2026-07-07T11:31:30Z
dc.descriptionWe point out that if heavy metastable particles composing the dark matter of our galaxy are responsible for the ultra-high energy cosmic rays (UHECR) then the leading tidal stream of the Sagittarius dwarf galaxy could be detected through UHECR. The signal would be an anisotropy in the UHECR flux smaller than the telltale anisotropy towards the galactic center that would first establish unstable dark matter as the origin of the UHECR.
dc.description14 pages, 5 figures, replaced with accepted version
dc.identifierhttps://arxiv.org/abs/hep-ph/0311001
dc.identifierhttp://arxiv.org/abs/hep-ph/0311001
dc.identifierPhys.Rev.D70:023010,2004
dc.identifierdoi:10.1103/PhysRevD.70.023010
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/197290
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDetectability of the Sgr Dwarf Leading Tidal Stream with Auger, EUSO or OWL
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