Pith Number
pith:B7XUVSAC
pith:2007:B7XUVSACXG3266R4LO7AXBWIMP
not attested
not anchored
not stored
refs pending
What is the optimum stellar rotation rate for a collapsar?
arxiv:astro-ph/0703032 v1 · 2007-03-01 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{B7XUVSACXG3266R4LO7AXBWIMP}
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
✓
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 | 2026-05-18T04:36:20.276208Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
0fef4ac802b9b7af7a3c5bbe0b86c863f4a8010a0beea7faf5be97cf33539a1a
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/B7XUVSACXG3266R4LO7AXBWIMP \
| 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: 0fef4ac802b9b7af7a3c5bbe0b86c863f4a8010a0beea7faf5be97cf33539a1a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "4fe541a8a54d8b2125ee3fcc438dc3eb652717cd177a27def5caa43c87458def",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2007-03-01T21:40:23Z",
"title_canon_sha256": "ee9db07b415f62ad4ea893e7526d862d02edae9c3a98ccb963bb1a71ccb010ea"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0703032",
"kind": "arxiv",
"version": 1
}
}