Pith Number
pith:YIQ6PSZW
pith:2017:YIQ6PSZWYK3B3BAERBJBDSD2VY
not attested
not anchored
not stored
refs pending
Radio Evolution of Supernova Remnants Including Non-linear Particle Acceleration: Insights from Hydrodynamic Simulations
arxiv:1711.06013 v2 · 2017-11-16 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{YIQ6PSZWYK3B3BAERBJBDSD2VY}
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 | 2026-05-18T00:26:14.288843Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c221e7cb36c2b61d8404885211c87aae16c10400d9cfca57aa3a82470eb70b50
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/YIQ6PSZWYK3B3BAERBJBDSD2VY \
| 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: c221e7cb36c2b61d8404885211c87aae16c10400d9cfca57aa3a82470eb70b50
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "58aa2d9caea17ebd1eda18ef28d1b0362daec8eeacf2ad789c370bd910f1c07c",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2017-11-16T10:32:12Z",
"title_canon_sha256": "7cb31a342749d11601abb5a6f904373e21c7f402a96dcf14ab43aa72e7060e1e"
},
"schema_version": "1.0",
"source": {
"id": "1711.06013",
"kind": "arxiv",
"version": 2
}
}