Pith Number
pith:KE2NOJR4
pith:2004:KE2NOJR4H6PXZEPUWJMYRF3DXR
not attested
not anchored
not stored
refs pending
Three-dimensional relativistic simulations of rotating neutron-star collapse to a Kerr black hole
arxiv:gr-qc/0403029 v2 · 2004-03-06 · gr-qc · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{KE2NOJR4H6PXZEPUWJMYRF3DXR}
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 | 2026-05-18T04:12:01.030550Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5134d7263c3f9f7c91f4b259889763bc771b45e141878cf7b232cbaae40b91ad
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KE2NOJR4H6PXZEPUWJMYRF3DXR \
| 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: 5134d7263c3f9f7c91f4b259889763bc771b45e141878cf7b232cbaae40b91ad
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "bb29d032bdaeaa2c74263a0f39368a20a070753477018150f9fa4b944192370a",
"cross_cats_sorted": [
"astro-ph"
],
"license": "",
"primary_cat": "gr-qc",
"submitted_at": "2004-03-06T14:25:11Z",
"title_canon_sha256": "cd587c8c1f470f34fbf9d468f14cb398775b8e21e078bb48d11b0876b2657cf3"
},
"schema_version": "1.0",
"source": {
"id": "gr-qc/0403029",
"kind": "arxiv",
"version": 2
}
}