  Using the synchronous coordinates, the creation of a Schwarzschild black hole
immersed in a de Sitter spacetime can be viewed as a coherent creation of a
collection of timelike geodesics. The previously supposed conical singularities
do not exist at the horizons of the constrained instan- ton. Instead, the
unavoidable irregularity is presented as a non-vanishing second fundamental
form elsewhere at the quantum transition 3-surface. The same arguments can be
applied to charged, topological or higher dimensional black hole cases.
