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

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

2003-10-31

arxiv.org/abs/hep-ph/0311001v2

Phys.Rev.D70:023010,2004

Physics

High Energy Physics

High Energy Physics - Phenomenology

14 pages, 5 figures, replaced with accepted version

Scientific paper

10.1103/PhysRevD.70.023010

We 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.

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