pith:YCPM75IM
Birth of Inflationary Universes via Wineglass Wormholes and their No-Boundary Relatives
Wineglass wormholes can nucleate inflationary spacetimes from asymptotically flat or AdS regions via analytic continuation.
arxiv:2605.10548 v2 · 2026-05-11 · hep-th · gr-qc
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Claims
We present explicit numerical wormhole solutions supported either by an axionic field or a magnetic gauge field, in both cases in conjunction with a self-interacting scalar field. In the limit of small axionic or magnetic charge, wineglass wormhole solutions split into two separate geometries, one being the background spacetime and the other a disconnected no-boundary instanton.
The analytic continuation from the Euclidean wineglass geometry to a Lorentzian expanding spacetime is valid and that the local maximum of the scale factor indeed triggers inflation after materialization.
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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| First computed | 2026-07-27T01:20:17.826102Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c09ecff50cd8c6035bbda67b216abf201b737e1900e33e07e18ef0c0ea79931d
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Canonical record JSON
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