Pith Number
pith:3V4HQAIV
pith:2011:3V4HQAIVRDILINCCL3QDB6SN23
not attested
not anchored
not stored
refs pending
Modeling supernova remnants: effects of diffusive cosmic-ray acceleration on the evolution, application to observations
arxiv:1105.5966 v1 · 2011-05-30 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{3V4HQAIVRDILINCCL3QDB6SN23}
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 | 2026-05-18T02:01:46.201582Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
dd7878011588d0b434425ee030fa4dd6fa9ed4af55a51d08b6768d100fd6f27c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/3V4HQAIVRDILINCCL3QDB6SN23 \
| 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: dd7878011588d0b434425ee030fa4dd6fa9ed4af55a51d08b6768d100fd6f27c
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a35bbfd8f83c3ddf4785fe88db65083d02518a1882b5686512debd1312b637e7",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2011-05-30T12:41:32Z",
"title_canon_sha256": "4a27d7099de138ec32e2a3cd4310918a2df7fff09c6ea39b0641132f5005831b"
},
"schema_version": "1.0",
"source": {
"id": "1105.5966",
"kind": "arxiv",
"version": 1
}
}