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A cosmological wave function describing the tunneling of the Universe from "nothing" into a de Sitter space is found in a simple minisuperspace model. The tunneling probability is proportional to exp (-38{G^2ₕ}), where ₕ is the vacuum energy density at an extremum of the effective potential V (). The tunneling is most probable to the highest maximum of V ().
Alexander Vilenkin (Sun,) studied this question.