Pith Number
pith:GWSQRH5X
pith:1999:GWSQRH5XSSVSJOCLHDDNH6JX26
not attested
not anchored
not stored
refs pending
Stability and collapse of rapidly rotating, supramassive neutron stars: 3D simulations in general relativity
arxiv:astro-ph/9911308 v1 · 1999-11-16 · astro-ph · gr-qc
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{GWSQRH5XSSVSJOCLHDDNH6JX26}
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 | 2026-07-04T16:11:54.698544Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
35a5089fb794ab24b84b38c6d3f937d78bfaae457ad136ee450be85414548f4c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/GWSQRH5XSSVSJOCLHDDNH6JX26 \
| 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: 35a5089fb794ab24b84b38c6d3f937d78bfaae457ad136ee450be85414548f4c
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "46934b1976d3ad1e2ea7bbc29ea42e0d4811b98b3ad2d324316dd78ec6545328",
"cross_cats_sorted": [
"gr-qc"
],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "1999-11-16T15:50:48Z",
"title_canon_sha256": "b76b0e3bbb43ceeb23fb303321ccb0d06948ee2075d8cc0701c5e567fe8b5968"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/9911308",
"kind": "arxiv",
"version": 1
}
}