pith:N2FFKGWV
A Tale of Two Hartle-Hawking Wave Functions: Fully Gravitational vs Partially Frozen
The phase in Hartle-Hawking wave functions arises only when the gravitational path integral fully integrates over boundary configurations rather than fixing them.
arxiv:2605.13970 v1 · 2026-05-13 · hep-th · gr-qc
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Claims
Our results suggest that the phase problem is controlled by whether the gravitational path integral is fully dynamical or partially frozen.
That the one-loop correction to the hyperbolic-ball partition function gives the leading contribution to the wave-function norm and that the boundary fluctuations are correctly captured by the chosen regularization.
In AdS the fully gravitational Hartle-Hawking wave function acquires a nontrivial one-loop phase while the partially frozen version stays real and positive; a partially frozen de Sitter sphere shows phase cancellation.
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Receipt and verification
| First computed | 2026-05-17T23:39:13.505186Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
6e8a551ad5d21d510221f94895ffc321f9d4dd3bf66f1fb7a1b90955b3b2d375
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/N2FFKGWV2IOVCARB7FEJL76DEH \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
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Canonical record JSON
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