  We will consider the least-order torsional completion of gravity for a
spacetime filled with fermionic Dirac matter fields, and we study the effects
of the background-induced non-linear potentials for the matter field themselves
in view of their effects for both standard models of physics: from the one of
cosmology to that of particles, we will discuss the mechanisms of generation of
the cosmological constant and particle masses as well as the phenomenology of
leptonic weak-like forces and neutrino oscillations, the problem of zero-point
energy, how there can be neutral massive fields as candidates for dark matter,
and avoidance of gravitational singularity formation; we will show the way in
which all these different effects can nevertheless be altogether described in
terms of just a single model, which will be thoroughly discussed in the end.

General Relativity and Quantum Cosmology