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

How is a Black Hole Created from Nothing?