Pith Number
pith:GJEZRAF5
pith:2017:GJEZRAF5ZH5LEAY4N5HQPP7G2D
not attested
not anchored
not stored
refs pending
Oscillation modes of rapidly rotating neutron stars in scalar-tensor theories of gravity
arxiv:1705.06984 v1 · 2017-05-19 · gr-qc · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{GJEZRAF5ZH5LEAY4N5HQPP7G2D}
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 | 2026-05-18T00:35:20.445309Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
32499880bdc9fab2031c6f4f07bfe6d0f7c5521012d54599829bfdd180f76748
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/GJEZRAF5ZH5LEAY4N5HQPP7G2D \
| 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: 32499880bdc9fab2031c6f4f07bfe6d0f7c5521012d54599829bfdd180f76748
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "1e959f2a658c2f48e96284142307e3efa8d6c3aa3e2b9b02fc43e8deebb48627",
"cross_cats_sorted": [
"astro-ph.HE"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "gr-qc",
"submitted_at": "2017-05-19T13:39:34Z",
"title_canon_sha256": "446d343543b9d4aa89cf9ac73ff1a0815a3e81179ac200419f6a64eb540208f9"
},
"schema_version": "1.0",
"source": {
"id": "1705.06984",
"kind": "arxiv",
"version": 1
}
}