pith:OTTQ2SLY
Quantum Field Theory of Black Hole Perturbations with Backreaction VI. Apparent Horizons, Quasi-Local Mass and Effective Classical Metrics
The apparent horizon of an evaporating black hole is determined to second order in perturbations, enabling reconstruction of a quantum-corrected effective metric.
arxiv:2605.13714 v1 · 2026-05-13 · gr-qc · astro-ph.HE
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Claims
We determine the shape of the apparent horizon to second order in the perturbations... taking expectation values of this metric, we obtain an effective classical metric, whose causal structure can then be visualised in a quantum corrected Penrose diagram.
The perturbative expansion truncated at second order remains valid for the dynamics of evaporating black holes, and the reduced phase space variables fully capture the relevant physics without higher-order terms or gauge artifacts dominating the horizon and metric reconstruction.
The apparent horizon shape is derived to second order for perturbed evaporating black holes, and an effective classical metric is obtained from quantum expectation values of the reconstructed spacetime.
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| First computed | 2026-05-18T02:44:16.722670Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
74e70d497892fbe32f75cad101bed7c092a9ce8c26173240f99a9b303dd2db96
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/OTTQ2SLYSL56GL3VZLIQDPWXYC \
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Canonical record JSON
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