Pith Number
pith:BJLU3QYL
pith:1997:BJLU3QYL57K3XQB4WRX3R5HVR5
not attested
not anchored
not stored
refs pending
Spontaneous symmetry breaking of rapidly rotating stars in general relativity: influence of the 3D-shift vector
arxiv:gr-qc/9710121 v1 · 1997-10-28 · gr-qc · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{BJLU3QYL57K3XQB4WRX3R5HVR5}
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 | 2026-05-18T04:21:31.864160Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
0a574dc30befd5bbc03cb46fb8f4f58f70671c2f057ae54935ae35e2412f6891
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/BJLU3QYL57K3XQB4WRX3R5HVR5 \
| 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: 0a574dc30befd5bbc03cb46fb8f4f58f70671c2f057ae54935ae35e2412f6891
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "28e03fb5f4715634882627844acae559be7fa5b76e055423b837679ee2de7cc9",
"cross_cats_sorted": [
"astro-ph"
],
"license": "",
"primary_cat": "gr-qc",
"submitted_at": "1997-10-28T14:53:38Z",
"title_canon_sha256": "c46f2b3d431fd3942d44639ab2410bf6352d8e8c3ae65b465f13817a0235cf7a"
},
"schema_version": "1.0",
"source": {
"id": "gr-qc/9710121",
"kind": "arxiv",
"version": 1
}
}