Pith Number
pith:FUP3U4H7
pith:2013:FUP3U4H7A5G6QLAOMAYUKUOHD5
not attested
not anchored
not stored
refs pending
Magnetic fields in Accretion Discs around Neutron Stars - Consequences for the change of spin
arxiv:1312.3941 v1 · 2013-12-13 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{FUP3U4H7A5G6QLAOMAYUKUOHD5}
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 | 2026-05-18T03:04:47.067559Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
2d1fba70ff074de82c0e60314551c71f73297673a9a2e15242f64e28f6585c20
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/FUP3U4H7A5G6QLAOMAYUKUOHD5 \
| 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: 2d1fba70ff074de82c0e60314551c71f73297673a9a2e15242f64e28f6585c20
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "1aea52e02cf0cb00f1703f32f3e0a4b1b51772962aab6d9af61be1299731dbea",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2013-12-13T20:59:47Z",
"title_canon_sha256": "50a3c52b1b1b72bedb30b90b240a4c816c96c0099aebf095a2a562d85e7d51f8"
},
"schema_version": "1.0",
"source": {
"id": "1312.3941",
"kind": "arxiv",
"version": 1
}
}