Pith Number
pith:3Q5QYFXI
pith:2020:3Q5QYFXIW6YT7U5QN3NIYRV3US
not attested
not anchored
not stored
refs pending
Can Lense-Thirring precession produce QPOs in supersonic accretion flows?
arxiv:2011.09032 v1 · 2020-11-18 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{3Q5QYFXIW6YT7U5QN3NIYRV3US}
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 | 2026-07-05T02:07:52.238307Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
dc3b0c16e8b7b13fd3b06eda8c46bba48340421fa13f1f4e143caa6f1b8e4999
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/3Q5QYFXIW6YT7U5QN3NIYRV3US \
| 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: dc3b0c16e8b7b13fd3b06eda8c46bba48340421fa13f1f4e143caa6f1b8e4999
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "4c027f6e6f343dbd820e7971d06100b6561d12b59a7c8f6acc3db50d32021493",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2020-11-18T01:38:33Z",
"title_canon_sha256": "806245cc3a88ffc56ae1231aedb0b1f3ca2e8717a782b34e3cafc9bc3f72d205"
},
"schema_version": "1.0",
"source": {
"id": "2011.09032",
"kind": "arxiv",
"version": 1
}
}