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On the Exponentially Large Probability of Transition through the Lavrelashvili-Rubakov-Tinyakov Wormhole

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arxiv gr-qc/9602049 v2 pith:R3K3M6BV submitted 1996-02-26 gr-qc hep-th

classification gr-qchep-th
keywords exponentiallywormholelargelavrelashvili-rubakov-tinyakovmodelprobabilitytransitionaction
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The model consisting of gravitational, scalar and axionic fields is considered. It is shown that the action of the Lavrelashvili-Rubakov-Tinyakov wormhole can be made arbitrarily negative by varying the parameters of the model. This means that semiclassically calculated probability of transition through this wormhole is not exponentially small (as usual) but exponentially large.

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  1. Birth of Inflationary Universes via Wineglass Wormholes and their No-Boundary Relatives

    hep-th 2026-05 unverdicted novelty 6.0 of 10

    Wineglass wormholes with a local maximum in the scale factor mediate the birth of inflationary spacetimes and split into background plus no-boundary geometries at small axionic or magnetic charge.

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