Nonsingularity in the no-boundary Universe

In the no-boundary Universe of Hartle and Hawking, the path integral for the quantum state of the Universe must be summed only over nonsingular histories. If the quantum corrections to the Hamilton-Jacobi equation in the interpretation of the wave packet is taken into account, then all classical trajectories should be nonsingular. The quantum behaviour of the classical singularity in the S-1 x S-m model (m greater than or equal to 2) is also clarified. II is argued that the Universe should evolve from the zero momentum state, instead from a zero volume state, to a 3-geometry state.