Pith Number
pith:R42DJJHO
pith:2022:R42DJJHOGYQHISDSPS3NV4WMZL
not attested
not anchored
not stored
refs pending
Generation of neutrino dark matter, baryon asymmetry, and radiation after quintessential inflation
arxiv:2210.05214 v1 · 2022-10-11 · hep-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{R42DJJHOGYQHISDSPS3NV4WMZL}
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
✓
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.
Cited by
Receipt and verification
| First computed | 2026-07-05T05:57:57.594289Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8f3434a4ee36207448727cb6daf2cccae5f3e4fe369f308aed237e3b3ebd8405
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/R42DJJHOGYQHISDSPS3NV4WMZL \
| 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: 8f3434a4ee36207448727cb6daf2cccae5f3e4fe369f308aed237e3b3ebd8405
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "543fdfcd94b4a438f7c0b36596d8de177e5484cf061e4881e7b515def01f8a49",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "hep-ph",
"submitted_at": "2022-10-11T07:31:10Z",
"title_canon_sha256": "0ea132910a82ec92fce9e3e85c5f539a4b58cd47f78ba1d8ff7d23a9ac20617e"
},
"schema_version": "1.0",
"source": {
"id": "2210.05214",
"kind": "arxiv",
"version": 1
}
}