pith:FHXHGYI4
Can Oscillatory and Persistent Nonlinearities Be Bridged in Black Hole Ringdown?
Quadratic quasinormal modes and the Christodoulou memory effect in black hole ringdown are linked by coefficients set by the remnant black hole parameters.
arxiv:2603.07469 v3 · 2026-03-08 · gr-qc
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Claims
We show that they are related through bridge coefficients which depend primarily on remnant black hole parameters during ringdown.
The assumption that the bridge coefficients are determined solely by remnant black hole parameters with no significant dependence on initial perturbation details or higher-order nonlinear terms.
Quadratic quasinormal modes and Christodoulou memory effect are related through bridge coefficients depending primarily on remnant black hole parameters.
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| First computed | 2026-05-21T01:04:24.256422Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
29ee73611ca9e110cb9d803bdf6422f922db7b2b94fd6eabc89f886a85d71a81
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/FHXHGYI4VHQRBS45QA556ZBC7E \
| 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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