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The power of Lorentzian wormholes

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arxiv 2302.01360 v1 pith:54OPTGFN submitted 2023-02-02 hep-th gr-qc

The power of Lorentzian wormholes

classification hep-th gr-qc
keywords lorentzianwormholescrotchesspacetimesevidencesemiclassicalactionarea
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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As shown by Louko and Sorkin in 1995, topology change in Lorentzian signature involves spacetimes with singular points, which they called crotches. We modify their construction to obtain Lorentzian semiclassical wormholes in asymptotically AdS. These solutions are obtained by inserting crotches on known saddles, like the double-cone or multiple copies of the Lorentzian black hole. The crotches implement swap-identifications, and are classically located at an extremal surface. The resulting Lorentzian wormholes have an instanton action equal to their area, which is responsible for topological suppression in any number of dimensions. We conjecture that including these Lorentzian wormhole spacetimes is gauge-equivalent to path integrating over all mostly Euclidean smooth spacetimes. We present evidence for this by reproducing semiclassical features of the genus expansion of the spectral form factor, and of a late-time two point function, by summing over the moduli space of Lorentzian wormholes. As a final piece of evidence, we discuss the Lorentzian version of West-Coast replica wormholes.

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Cited by 2 Pith papers

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  2. Some universalities in the partition functions of low-dimensional gravity models

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    Conjectures universalities in partition functions across low-dimensional gravity models by examining similarities under parameter changes, wavefunction behaviors, entanglement, and wormhole connections.