Pith Number
pith:K3K5PZVK
pith:2016:K3K5PZVKRD4U4GLQJ5MVYGPBUY
not attested
not anchored
not stored
refs pending
Magnetorotational dynamo chimeras. The missing link to turbulent accretion disk dynamo models?
arxiv:1607.02903 v1 · 2016-07-11 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{K3K5PZVKRD4U4GLQJ5MVYGPBUY}
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 | 2026-05-18T00:51:16.924704Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
56d5d7e6aa88f94e19704f595c19e1a63241620c41c88954d234dacf2d2d11c4
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/K3K5PZVKRD4U4GLQJ5MVYGPBUY \
| 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: 56d5d7e6aa88f94e19704f595c19e1a63241620c41c88954d234dacf2d2d11c4
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "70372d37f1fe75b11c201571f13a8527669a049149a24fc277af3632585d6053",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2016-07-11T11:14:04Z",
"title_canon_sha256": "148fa6a92d330ea447db11344e8e41cf0aa2ea79bf757f599e8b99c87f3bc067"
},
"schema_version": "1.0",
"source": {
"id": "1607.02903",
"kind": "arxiv",
"version": 1
}
}