Pith Number
pith:35YQPFA5
pith:2010:35YQPFA5MDTXCCHIJFJIABCMAE
not attested
not anchored
not stored
refs pending
Evolution of white dwarf stars with high-metallicity progenitors: the role of 22Ne diffusion
arxiv:1006.4170 v1 · 2010-06-21 · astro-ph.SR · physics.plasm-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{35YQPFA5MDTXCCHIJFJIABCMAE}
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 | 2026-05-18T02:06:43.898555Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
df7107941d60e77108e8495280044c0109bb2687805b3875e64be157051c5ec0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/35YQPFA5MDTXCCHIJFJIABCMAE \
| 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: df7107941d60e77108e8495280044c0109bb2687805b3875e64be157051c5ec0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "fe8538a4c72d9452f63e37658e0788ba8a789d7639576f04d303079f31ba54c2",
"cross_cats_sorted": [
"physics.plasm-ph"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2010-06-21T20:24:23Z",
"title_canon_sha256": "2885d3a8e4c7e06fbbc013d256680565999fadca1b98ca752fce24f807af0d69"
},
"schema_version": "1.0",
"source": {
"id": "1006.4170",
"kind": "arxiv",
"version": 1
}
}