Pith Number
pith:WLPCECNJ
pith:2001:WLPCECNJUEUR2URL3GZJKUFZ37
not attested
not anchored
not stored
refs pending
Frequencies of f-modes in differentially rotating relativistic stars and secular stability limits
arxiv:gr-qc/0112017 v3 · 2001-12-10 · gr-qc · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{WLPCECNJUEUR2URL3GZJKUFZ37}
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
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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 | 2026-07-04T16:26:59.900585Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b2de2209a9a1291d522bd9b29550b9dfe9efa9bdd0d85d14a38fdad905c347b1
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/WLPCECNJUEUR2URL3GZJKUFZ37 \
| 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: b2de2209a9a1291d522bd9b29550b9dfe9efa9bdd0d85d14a38fdad905c347b1
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "761373a8a15839dc473a8c81cbc6207e56a3d6c9e2df27316bfc0b784b896fbe",
"cross_cats_sorted": [
"astro-ph"
],
"license": "",
"primary_cat": "gr-qc",
"submitted_at": "2001-12-10T14:31:19Z",
"title_canon_sha256": "ff10087187618de43e93db4ca879aeae5cc9c126f74f98b6a024729bbade5f71"
},
"schema_version": "1.0",
"source": {
"id": "gr-qc/0112017",
"kind": "arxiv",
"version": 3
}
}