  We computed a new set of static fission properties suited for r-process
calculations. The potential energy surfaces and collective inertias of 3640
nuclei in the superheavy region are obtained from Self-Consistent Mean-Field
calculations using the Barcelona-Catania-Paris-Madrid energy density
functional. The fission path is computed as a function of the quadrupole moment
by minimizing the potential energy and exploring octupole and hexadecapole
deformations. The spontaneous fission lifetimes are evaluated employing
different schemes for the collective inertias and vibrational energy
corrections. This allows to explore the sensitivity of the lifetimes to those
quantities together with the collective ground state energy along the
superheavy landscape. We computed neutron induced stellar reaction rates
relevant for r-process nucleosynthesis using the statistical approach and study
the impact of collective inertias. The competition between different reaction
channels including neutron induced rates, spontaneous fission and alpha decay
is discussed for typical r-process conditions.
