Pith Number
pith:RY6555Y3
pith:2012:RY6555Y32U4ZIVL5PURUNJP2RU
not attested
not anchored
not stored
refs pending
Hall drift in the crust of neutron stars - necessary for radio pulsar activity?
arxiv:1206.1790 v1 · 2012-06-08 · astro-ph.SR · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{RY6555Y32U4ZIVL5PURUNJP2RU}
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
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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 | 2026-05-18T03:53:55.457464Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8e3ddef71bd53994557d7d2346a5fa8d26c78d83d7aef2e9b097629a223b17df
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/RY6555Y32U4ZIVL5PURUNJP2RU \
| 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: 8e3ddef71bd53994557d7d2346a5fa8d26c78d83d7aef2e9b097629a223b17df
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "18d9d96d3aaf51f67160ece169b571b69b71d09dd9a0a29191ce1f08ed0ef3d5",
"cross_cats_sorted": [
"astro-ph.HE"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2012-06-08T15:15:24Z",
"title_canon_sha256": "3c4c38f9dc1569d78d8a4e0a84daebf6b232e3bb2e27497c92af112b5d105207"
},
"schema_version": "1.0",
"source": {
"id": "1206.1790",
"kind": "arxiv",
"version": 1
}
}