Introduction
The quantum states of Universe as modes of classical spinor field in the "world of classical worlds"
WCW Kähler metric from Kähler function
WCW Kähler metric from symmetries
WCW Kähler metric as anticommutators of supersymplectic super Noether charges
What principle selects the preferred extremals?
WCW
Basic notions
Constraints on WCW geometry
Identification of the Kähler function
Definition of Kähler function
The values of the Kähler coupling strength?
What principle selects the preferred extremals?
Why nonlocal Kähler function?
Some properties of Kähler action
Vacuum degeneracy and some of its implications
Fourdimensional General Coordinate Invariance
WCW geometry, generalized catastrophe theory, and phase transitions
