Pith Number
pith:6KXZZQNB
pith:2012:6KXZZQNBJJNXLS3MWEWYSB5HXB
not attested
not anchored
not stored
refs pending
Can Zee-Babu model implemented with scalar dark matter explain both Fermi-LAT 130 GeV $\gamma$-ray excess and neutrino physics ?
arxiv:1209.1685 v3 · 2012-09-08 · hep-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{6KXZZQNBJJNXLS3MWEWYSB5HXB}
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 | 2026-05-18T02:54:21.734088Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
f2af9cc1a14a5b75cb6cb12d8907a7b8792a490a20be7d0a6a915cb104f9667d
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/6KXZZQNBJJNXLS3MWEWYSB5HXB \
| 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: f2af9cc1a14a5b75cb6cb12d8907a7b8792a490a20be7d0a6a915cb104f9667d
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "1945f12ef2ba35485f00836697d185e91de5571b1a916cb51bca175f25640cb3",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "hep-ph",
"submitted_at": "2012-09-08T03:42:26Z",
"title_canon_sha256": "b221ef1fd36eb142c3958d862c01f64f1021a2bff28b07982fd8c5e729182ecf"
},
"schema_version": "1.0",
"source": {
"id": "1209.1685",
"kind": "arxiv",
"version": 3
}
}