Pith Number
pith:IIP7CYIG
pith:2007:IIP7CYIGJRUXEYTKKPES47IHJC
not attested
not anchored
not stored
refs pending
LNRF-velocity hump-induced oscillations of a Keplerian disc orbiting near-extreme Kerr black hole: A possible explanation of high-frequency QPOs in GRS 1915+105
arxiv:0704.1252 v2 · 2007-04-10 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{IIP7CYIGJRUXEYTKKPES47IHJC}
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.
Cited by
Receipt and verification
| First computed | 2026-07-04T17:03:14.899935Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
421ff161064c6972626a53c92e7d07489fbc14d6db450c3e73b550ed02b71841
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/IIP7CYIGJRUXEYTKKPES47IHJC \
| 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: 421ff161064c6972626a53c92e7d07489fbc14d6db450c3e73b550ed02b71841
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "dd45960be89c9dd0a62d62e4ca5ac0c1ea0fa6740ce3aa13384c07c3acf070a1",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2007-04-10T18:57:32Z",
"title_canon_sha256": "d3fbf898d8740e8ae00d9866ce0bc2c31a279500ce73985c4da58e4ba06d1d10"
},
"schema_version": "1.0",
"source": {
"id": "0704.1252",
"kind": "arxiv",
"version": 2
}
}