2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/46601Neutrino 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.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 1996High Energy Physics - Phenomenologytext