Pith Number
pith:54HZ4ZQD
pith:2024:54HZ4ZQD35T7WWEWUIQHX5FA7V
not attested
not anchored
not stored
refs pending
Could the neutrino emission of TXS 0506+056 come from the accretion flow of the supermassive black hole?
arxiv:2411.17632 v4 · 2024-11-26 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{54HZ4ZQD35T7WWEWUIQHX5FA7V}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge
Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
Author claim
· sign in to
claim
4
Citations
5
Replications
✓
Portable graph bundle live · download bundle · merged
state
The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same
current state with the deterministic merge algorithm.
Receipt and verification
| First computed | 2026-07-05T10:04:41.103650Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
ef0f9e6603df67fb5896a2207bf4a0fd5f54609f6d3b6e30047b46b9bb06a920
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/54HZ4ZQD35T7WWEWUIQHX5FA7V \
| 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: ef0f9e6603df67fb5896a2207bf4a0fd5f54609f6d3b6e30047b46b9bb06a920
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "562fe9fce0afb75e9daa04de0e72cddc8ff894151d9e1d67b639aa1a602fec61",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by-nc-sa/4.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2024-11-26T17:44:16Z",
"title_canon_sha256": "320b4f07b5dc6c38476875e2c55398347cb8c0caa91d526d792bd301139d806a"
},
"schema_version": "1.0",
"source": {
"id": "2411.17632",
"kind": "arxiv",
"version": 4
}
}