A Study of the Behavior of Ultra-High Energy Neutrinos

Abstract

Neutrino Oscillations in the presence of strong gravitational fields are studied specifically for Majorana neutrinos. We look at ultra high energy neutrinos $(\sim 1$ PeV) emanating from Active Galactic Nuclei (AGN). Fluxes of different flavor neutrinos are estimated and probabilities for different neutrino transitions calculated.

Comments: 3 pages, uses sprocl.sty, To be published in the proceedings of 1996 Annual Divisional Meeting (DPF96) of the Division of Particles and Fields of the American Physical Society, Minneapolis, MN, 10-15 Aug 1996