  Black hole accretion disks have been proposed as good candidates for a range
of interesting nucleosynthesis, including the r-process. The presence of the
black hole influences the neutrino fluxes and affects the nucleosynthesis
resulting from the interaction of the emitted neutrinos and hot outflowing
material ejected from the disk. We study the impact of general relativistic
effects on the neutrinos emitted from black hole accretion disks. We present
abundances obtained by considering null geodesics and energy shifts for two
different disk models. We find that both the bending of the neutrino
trajectories and the energy shifts have important consequences for the
nucleosynthetic outcome
