Bounds on Dark Matter from the ``Atmospheric Neutrino Anomaly''
J. M. LoSecco
Abstract
Bounds are derived on the cross section, flux and energy density of new particles that may be responsible for the atmospheric neutrino anomaly. 4.6 × 10-45 cm2 < σ<2.4 × 10-34 cm2 Decay of primordial homogeneous dark matter can be excluded.
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