  Two major recent developments in theory and computational resources created
the favorable conditions for achieving a microscopic description of nuclear
fission almost eighty years after its discovery in 1939 by Hahn and Strassmann
(1930). The first major development was in theory, the extension of the
Time-Dependent Density Functional Theory (TDDFT) to superfluid fermion systems.
The second development was in computing, the emergence of powerful enough
supercomputers capable of solving the complex systems of equations describing
the time evolution in three dimensions without any restrictions of hundreds of
strongly interacting nucleons. Even though the available nuclear energy density
functionals (NEDFs) are phenomenological still, their accuracy is improving
steadily and the prospects of being able to perform calculations of the nuclear
fission dynamics and to predict many properties of the fission fragments,
otherwise not possible to extract from experiments, are within reach, all
without making recourse anymore to uncontrollable assumptions and simplified
phenomenological models.

Nuclear Theory