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hep-ph2003

Inconsistencies in Interpreting the Atmospheric Neutrino Anomaly

John M. LoSecco

We note a discrepancy between the value of R expected on the basis of the muon neutrino angular distribution and the value actually observed. The energy independence of leads t…

hep-ph2000

Bounds on Extra Dimensions from Binary Pulsars

J. M. LoSecco

Evidence for gravitational radiation from binary pulsars places constraints on properties of ``large'' extra dimensions. The size of these extra dimensions must exceed about 37 AU…

hep-ph1999

Atmospheric Neutrinos: Past, Present and

John M. LoSecco

This paper reviews the history of the atmospheric neutrino anomaly. The historical record does not support more recent claims that the anomaly constitutes evidence for a neutrino m…

hep-ph1999

Possible Sources of a Transient Natural Neutrino Flux

J. M. LoSecco

Recent observations of variability in the ``atmospheric neutrino'' rate place constraints on possible explanations of the atmospheric neutrino anomaly. Many proposed solutions to t…

hep-ph1998

What the Atmospheric Neutrino Anomaly is Not

J. M. LoSecco

The atmospheric neutrino anomaly is the apparent reduction of the ratio observed in underground detectors. It represents either a reduction in the muon neutrino interac…

hep-ph1998

Problems with Atmospheric Neutrino Oscillations

J. M. LoSecco

The neutrino oscillation hypothesis does a poor job of representing the atmospheric neutrino anomaly. The anomaly is observed over 4 decades in path length and at least a factor of…