Pith Number
pith:OACZ2ZQO
pith:2015:OACZ2ZQOIDFLPHCNRHMBW6E5D5
not attested
not anchored
not stored
refs pending
Should One Use the Ray-by-Ray Approximation in Core-Collapse Supernova Simulations?
arxiv:1512.00113 v2 · 2015-12-01 · astro-ph.SR · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{OACZ2ZQOIDFLPHCNRHMBW6E5D5}
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 | 2026-05-18T00:59:58.933940Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
70059d660e40cab79c4d89d81b789d1f45054b43e7c4dd20e04a6d1c76a9fb9a
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/OACZ2ZQOIDFLPHCNRHMBW6E5D5 \
| 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: 70059d660e40cab79c4d89d81b789d1f45054b43e7c4dd20e04a6d1c76a9fb9a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "8980b5e048b6dbfc99856cf2339094631c8730caf96109e21bc691f149b03702",
"cross_cats_sorted": [
"astro-ph.HE"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2015-12-01T01:13:28Z",
"title_canon_sha256": "23afd6b2b9f1c3779d114af79cac898cf87020a011aaa0e1f017bd77df5e76b0"
},
"schema_version": "1.0",
"source": {
"id": "1512.00113",
"kind": "arxiv",
"version": 2
}
}