Detectability of the Sgr Dwarf Leading Tidal Stream with Auger, EUSO or OWL
arXiv:hep-ph/0311001 · doi:10.1103/PhysRevD.70.023010
Abstract
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.
arXiv comment14 pages, 5 figures, replaced with accepted version
References in corpus (14)
- A 2MASS All-Sky View of the Sagittarius Dwarf Galaxy: I. Morphology of the Sagittarius Core and Tidal Arms
- Extension of the Cosmic-Ray Energy Spectrum Beyond the Predicted Greisen-Zatsepin-Kuz'min Cutoff
- Ultra-high energy cosmic rays without GZK cutoff
- The Kinematics, Orbit, and Survival of the Sagittarius Dwarf Spheroidal Galaxy
- Extremely high energy cosmic rays from relic particle decays
- Sagittarius Tidal Debris 90 kpc from the Galactic Center
- Ultra high energy cosmic rays and the large scale structure of the galactic magnetic field
- The Effects of the Sagittarius Dwarf Tidal Stream on Dark Matter Detectors
- Signatures of Topological Defects
- The toes of the ultra high energy cosmic ray spectrum
- Fragmentation functions in SUSY QCD and UHECR spectra produced in top-down models
- Monte Carlo simulation for jet fragmentation in SUSY-QCD
- Galactic Anisotropy as Signature of ``Top-Down'' Mechanisms of Ultra-High Energy Cosmic Rays
- Deflection of ultra high energy cosmic rays by the galactic magnetic field: from the sources to the detector