Pith Number
pith:OHV4RL6L
pith:1999:OHV4RL6LUYD6UZTYSGSCZ4LVC3
not attested
not anchored
not stored
refs pending
The evolution of circular, non-equatorial orbits of Kerr black holes due to gravitational-wave emission
arxiv:gr-qc/9910091 v3 · 1999-10-26 · gr-qc · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{OHV4RL6LUYD6UZTYSGSCZ4LVC3}
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.
Cited by
Receipt and verification
| First computed | 2026-05-18T02:37:27.874681Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
71ebc8afcba607ea667891a42cf17516f32864ae5ed7f1e17071be1f2ec63f91
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/OHV4RL6LUYD6UZTYSGSCZ4LVC3 \
| 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: 71ebc8afcba607ea667891a42cf17516f32864ae5ed7f1e17071be1f2ec63f91
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "08f10d4e16e6ea9efb0cb844ded8f8bdfbd24326d67a5310ba7e0ed2286c4672",
"cross_cats_sorted": [
"astro-ph"
],
"license": "",
"primary_cat": "gr-qc",
"submitted_at": "1999-10-26T18:32:02Z",
"title_canon_sha256": "caf354a9c23c4b60cf1abdd9bd48422124770f6d1ca2d67bc6cc9debf77fc9b8"
},
"schema_version": "1.0",
"source": {
"id": "gr-qc/9910091",
"kind": "arxiv",
"version": 3
}
}