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

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

1996-02-26

arxiv.org/abs/gr-qc/9602049v2

Phys.Lett. B381 (1996) 45-48

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

9 pages and 1 figure in LaTeX; there is some refinement in text; the title has been changed; the figure is added to the LaTeX

Scientific paper

10.1016/0370-2693(96)00563-1

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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