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Wormhole Nucleation from Anti-de Sitter vs Tryon Vacuum Fluctuation
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Wormhole Nucleation from Anti-de Sitter Speculative | Tryon Vacuum Fluctuation Historical | |
|---|---|---|
| Proposed | 2024 / 2026 | 1973 |
| Key figures | Panos Betzios, Olga Papadoulaki, George Lavrelashvili, Jean-Luc Lehners | Edward Tryon |
| In one sentence | A wave function for the universe in which a Euclidean wormhole, anchored in an anti-de Sitter region, gives birth to an expanding universe that begins with inflation. | Tryon's 1973 Nature paper proposed the universe is a quantum fluctuation with zero net energy, the historical precursor to all "universe from nothing" proposals. |
| Predictions |
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| Where it breaks |
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| Key unresolved problem | Which beginning wins: the wormhole, or the no-boundary instanton it turns into at zero charge. Current calculations still favour no-boundary overall, so the wormhole route needs a reason to be selected. | The pre-existing vacuum problem: Tryon's proposal still starts from a quantum vacuum that already comes with physical laws and geometry, so it explains the universe but not where those prior ingredients came from. |
| Reader vote | No votes yet | No votes yet |
Wormhole Nucleation from Anti-de Sitter
2024 / 2026 · Speculative
Tryon Vacuum Fluctuation
1973 · Historical
Proposed
2024 / 2026
1973
Key figures
Panos Betzios, Olga Papadoulaki, George Lavrelashvili, Jean-Luc Lehners
Edward Tryon
In one sentence
A wave function for the universe in which a Euclidean wormhole, anchored in an anti-de Sitter region, gives birth to an expanding universe that begins with inflation.
Tryon's 1973 Nature paper proposed the universe is a quantum fluctuation with zero net energy, the historical precursor to all "universe from nothing" proposals.
Predictions
- A small shift and faint oscillations in the [[cosmic microwave background]] on the largest angular scales, with a size set by the wormhole's charge
- Short-wavelength fluctuations identical to those of standard inflation, so the signature appears only on the largest scales
- Wormholes with small charge give a longer phase of inflation than wormholes with large charge
- Total energy of universe ~ 0
- Universes can spontaneously fluctuate from vacuum
Where it breaks
- Lavrelashvili and Lehners find that no-boundary instantons still dominate the overall probability, which weakens the case that wormholes are the preferred beginning.
- The universe needs a parent anti-de Sitter or flat region to emerge from, which moves the question of origins back one step.
- The predicted signal sits on the largest scales of the sky, where there are too few independent patches to measure it precisely.
- Tryon's proposal still presupposes a quantum vacuum and laws, not truly nothing
- Vilenkin (1982) provides the rigorous framework Tryon lacked
Key unresolved problem
Which beginning wins: the wormhole, or the no-boundary instanton it turns into at zero charge. Current calculations still favour no-boundary overall, so the wormhole route needs a reason to be selected.
The pre-existing vacuum problem: Tryon's proposal still starts from a quantum vacuum that already comes with physical laws and geometry, so it explains the universe but not where those prior ingredients came from.
Reader vote
No votes yet
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