Pith Number
pith:WDL4K6D4
pith:2016:WDL4K6D4N3ZBR6NN6OSKFXBMS3
not attested
not anchored
not stored
refs pending
Energy Spectrum of Fast Second Order Fermi Accelerators as Sources of Ultra-High-Energy Cosmic Rays
arxiv:1612.03675 v2 · 2016-12-12 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{WDL4K6D4N3ZBR6NN6OSKFXBMS3}
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 | 2026-05-18T00:15:30.946334Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b0d7c5787c6ef218f9adf3a4a2dc2c96f3e3856a09f5333250e15efa4e265c04
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/WDL4K6D4N3ZBR6NN6OSKFXBMS3 \
| 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: b0d7c5787c6ef218f9adf3a4a2dc2c96f3e3856a09f5333250e15efa4e265c04
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3485c56ed976b850c59d6a235add41b7526088acf26688a7986372fdae2b85a1",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2016-12-12T13:50:48Z",
"title_canon_sha256": "3970279e80365881f34deb8cb4b0d42f5e4a046817c6ccf4a8ca277467f73f18"
},
"schema_version": "1.0",
"source": {
"id": "1612.03675",
"kind": "arxiv",
"version": 2
}
}