Scalar-gravitational hamiltonian in the relativistic gravitation theory with logunov relations

It is shown that within the relativistic gravitation theory with Logunov relations, the scalar-gravitational Hamiltonian is nonzero, which automatically solves the problem of time in quantum geometrodynamics and allows us to construct a quantum theory of the Big Bang in the form of theory of the LemaItre primordial atom based on the Logunov concept asymptotically combined with the Gliner' idea of material interpretation of the cosmological constant in the classical potential form. Within the Hilbert-Einstein tensor-geometrical gravitation theory, the Hamiltonian is zero and this results in the time independence of the wave function of the Universe, which, in turn, does not allow to construct an atomic model of the Big Bang.