Pith Number
pith:G6LMMYG2
pith:2025:G6LMMYG25FTLRYJJJDI63PFAQS
not attested
not anchored
not stored
refs pending
Impact of Cosmic Ray Distribution on the Growth and Saturation of Bell Instability
arxiv:2511.21154 v2 · 2025-11-26 · astro-ph.HE · physics.plasm-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{G6LMMYG25FTLRYJJJDI63PFAQS}
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 | 2026-06-09T01:05:11.004984Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3796c660dae966b8e12948d1edbca08496eedbeaf839176b6c0c8b5abcd9a316
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/G6LMMYG25FTLRYJJJDI63PFAQS \
| 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: 3796c660dae966b8e12948d1edbca08496eedbeaf839176b6c0c8b5abcd9a316
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "600ac5599472a067f0d45ffd6875119cbf0039df474c47dd9687c04e87a31b15",
"cross_cats_sorted": [
"physics.plasm-ph"
],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2025-11-26T08:14:02Z",
"title_canon_sha256": "97631a06499afeba9f75a590c363e3b4f27bedd7ffc41a571f41701295ecfc8c"
},
"schema_version": "1.0",
"source": {
"id": "2511.21154",
"kind": "arxiv",
"version": 2
}
}