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Pith Number

pith:GJHV52G4

pith:2026:GJHV52G463GUZ6UXWUXHBDPJ6K
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TeV Gamma-Rays from the Low-Luminosity Active Galactic Nucleus NGC 4278: Implications for the Diffuse Neutrino Background

Chengchao Yuan, Ruo-Yu Liu

Lepto-hadronic winds in low-luminosity AGN can explain the PeV diffuse neutrino background once the local density is corrected for a TeV duty cycle of order 10^{-5}.

arxiv:2601.21411 v2 · 2026-01-29 · astro-ph.HE · astro-ph.GA

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Record completeness

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2 Internet Archive
3 Author claim open · sign in to claim
4 Citations open
5 Replications open
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Claims

C1strongest claim

a lepto-hadronic wind scenario can account for the PeV diffuse neutrino background when adopting a local LLAGN density (n_L,0) corrected for the TeV duty cycle (ΔT_TeV/T) ~ 10^{-5} Mpc^{-3}, as inferred from the LHAASO detection.

C2weakest assumption

That the observed TeV emission is produced by lepto-hadronic processes in sub-relativistic winds rather than leptonic jets, and that the single-source LHAASO detection can be used to infer a population-wide duty-cycle-corrected density that directly scales to the diffuse neutrino background.

C3one line summary

Lepto-hadronic winds in LLAGNs like NGC 4278 can account for the PeV diffuse neutrino background with a duty-cycle-corrected local density of ~10^{-5} Mpc^{-3} inferred from LHAASO data.

Formal links

2 machine-checked theorem links

Receipt and verification
First computed 2026-05-20T00:01:39.363798Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

324f5ee8dcf6cd4cfa97b52e708de9f286c6c67a2f1147e463c9674ac08cbef4

Aliases

arxiv: 2601.21411 · arxiv_version: 2601.21411v2 · doi: 10.48550/arxiv.2601.21411 · pith_short_12: GJHV52G463GU · pith_short_16: GJHV52G463GUZ6UX · pith_short_8: GJHV52G4
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/GJHV52G463GUZ6UXWUXHBDPJ6K \
  | 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: 324f5ee8dcf6cd4cfa97b52e708de9f286c6c67a2f1147e463c9674ac08cbef4
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "1e4c6127129b57dc563f04d69eeb22259c21aa1c18d9438c1cf0759d175e54da",
    "cross_cats_sorted": [
      "astro-ph.GA"
    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.HE",
    "submitted_at": "2026-01-29T08:50:14Z",
    "title_canon_sha256": "5f345fd5e7d4cecbd5c2ab28c84369344a2d2142bf50bc3fe74d14057c4e7cc5"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2601.21411",
    "kind": "arxiv",
    "version": 2
  }
}