Bounds on Dark Matter from the ``Atmospheric Neutrino Anomaly''

Details Bounds on Dark Matter from the ``Atmospheric Neutrino Anomaly'' Bounds on Dark Matter from the ``Atmospheric Neutrino Anomaly''

1997-06-16

arxiv.org/abs/hep-ph/9706368v1

Phys.Rev. D56 (1997) 4416-4418

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, TeX (revtex)

Scientific paper

10.1103/PhysRevD.56.4416

Bounds are derived on the cross section, flux and energy density of new
particles that may be responsible for the atmospheric neutrino anomaly. $4.6
\times 10^{-45} cm^2 < \sigma <2.4 \times 10^{-34} cm^2$ Decay of primordial
homogeneous dark matter can be excluded.

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