  We describe how physical universes that are composed of gauge and
gravitationally interacting bosonic and fermionic quantum fields arise from the
generic discrete distribution of many quantifiable properties of arbitrary
static entities. Alternate presentations of the smooth coarse-graining (fit)
for this discrete distribution compose probability-related evolving wave
function of the fields' dynamical modes. Their gauge modes, being symmetry
transformations, and constrained modes require no additional material
structure. We prove that evolution of any origin for which the quantum
superposition principle is absolute cannot be governed by specific laws. In
contrast, locally supersymmetric quantum fields that emerge as described from
the basic discrete distribution evolve by unchanging and closed physical laws.
The emergent quantum evolution is many-world; yet its Everett's branches whose
norm diminishes below a positive threshold cease to exist. Then some
experiments that for the standard Everett view would seem safe are instead
fatal for the participants. The Born rule arises dynamically in emergent
systems with extended regular past. It and, consequently, quasi-deterministic
macroscopic evolution emerge in systems that allow cosmological inflation but
not in typical random ones. This resolves the Boltzmann brain problem. We
explain how inflation creates new physical degrees of freedom around the Planck
scale. Quantum entanglement for the emergent fields is trivial because their
wave function, up to its representation, is material.
