pith:UOP5GCKC
Intermittent Turbulence, Fast Flavor Conversion, and Observable Supernova Probes
Intermittent turbulence in supernovae sets the fast flavor conversion fraction while neutrino spectral hierarchy fixes the sign of heating corrections.
arxiv:2601.11272 v3 · 2026-01-16 · astro-ph.HE
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Claims
Thus intermittency mainly controls the conversion fraction, while the neutrino spectral hierarchy controls the sign of the heating correction.
The assumption that the matter-noise memory kernel is generated by a finite She-Leveque log-Poisson cascade and that the marginal FFC channel projects onto this kernel to give a causal Volterra equation whose non-Markovian memory closes into a finite local system.
Using a She-Leveque cascade for intermittent turbulence in supernovae, the model predicts a fast flavor conversion fraction of approximately 0.455 and heating corrections of 4-6% whose sign depends on the neutrino spectral hierarchy.
References
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| First computed | 2026-05-18T03:09:24.418868Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/UOP5GCKCTUYBLOEZAPSJSBK3BN \
| 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())"
# expect: a39fd309429d3015b89903e499055b0b717b0c3513f7088a7d805846a2a7e5f8
Canonical record JSON
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