Pith Number
pith:KM6DQYDB
pith:2000:KM6DQYDB5OLDMKVXXYUTRLWIPN
not attested
not anchored
not stored
refs pending
Comment on ``Neutrino oscillations in the early universe: how can large lepton asymmetry be generated?"
arxiv:hep-ph/0008245 v3 · 2000-08-23 · hep-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{KM6DQYDB5OLDMKVXXYUTRLWIPN}
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
· sign in to
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.
Receipt and verification
| First computed | 2026-05-18T04:21:31.751912Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
533c386061eb96362ab7be2938aec87b74ec5ce2af2e594c353233f9b3489e8c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KM6DQYDB5OLDMKVXXYUTRLWIPN \
| 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: 533c386061eb96362ab7be2938aec87b74ec5ce2af2e594c353233f9b3489e8c
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "1eb5794a9eb97419c597646a661837227ac75a3dd7cf7f6f8e8a72be08c5a307",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "hep-ph",
"submitted_at": "2000-08-23T14:59:06Z",
"title_canon_sha256": "3220c8b4d04c8e28ca650e6c04f1e81967aa67cb110b9fe551f66ee8698c91f2"
},
"schema_version": "1.0",
"source": {
"id": "hep-ph/0008245",
"kind": "arxiv",
"version": 3
}
}