Bounds are derived on the cross section, flux and energy density of new particles that may be responsible for the atmospheric neutrino anomaly. 4.6×10−45cm2<σ<2.4×10−34cm2 Decay of primordial homogeneous dark matter can be excluded.
Cite
@article{arxiv.hep-ph/9706368,
title = {Bounds on Dark Matter from the ``Atmospheric Neutrino Anomaly''},
author = {J. M. LoSecco},
journal= {arXiv preprint arXiv:hep-ph/9706368},
year = {2014}
}