  Neutrinos are copiously emitted from black hole accretion disks playing a
fundamental role in their evolution, as well as in the production of gamma ray
bursts and r-process nucleosynthesis. The black hole generates a strong
gravitational field able to change the properties of the emerging neutrinos. We
study the influence of the black hole spin on the structure of the neutrino
surfaces, neutrino luminosities, average neutrino energies, and event counts at
SuperK. We consider several disk models and provide estimates that cover
different black hole efficiency scenarios. We discuss the influence of the
detector's inclination with respect to the axis of the torus on neutrino
properties. We find that tori around spinning black holes have larger
luminosities, energies and rates compared to tori around static black holes,
and that the inclination of the observer causes a reduction in the luminosities
and detection rates but an increase in the average energies.
