  The production and propagation of light antimatter nuclei has been calculated
using inclusive antiproton production cross sections from a new data analysis,
and coalescence models for the production of composite particles. Particles
were propagated using recently proven phenomenological approaches. The
atmospheric secondary flux is evaluated for the first time. The Galactic flux
obtained are larger than those obtained previously in similar calculations. The
non-annihilating scattering contributions of the propagated particles are
introduced. The preliminary results are shown and discussed.
