Abstract:
The dynamics of a spatially closed universe is studied in gravitation theory by means of the eigenfunctions and eigenvalues of the $3D$ projection of the Dirac operator. In a gauge that we call the Ashtekar gauge and construct by using an eigenfunction of this operator, the $3D$ volume of a spatial section is a canonical parameter, and the energy is a positive-definite functional of the dynamical variables (on the region of the phase space in which $\dot V>0$) proportional to the corresponding eigenvalue. There is a discrete set of frames of reference distinguished in this manner.