Pith Number
pith:4ZV2B36E
pith:2012:4ZV2B36ENUHZQMPE4ZN2U7LSIY
not attested
not anchored
not stored
refs pending
Non-Gaussianity in the Cosmic Microwave Background Induced by Dipolar Dark Matter
arxiv:1210.4106 v2 · 2012-10-15 · gr-qc · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{4ZV2B36ENUHZQMPE4ZN2U7LSIY}
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.
Receipt and verification
| First computed | 2026-05-18T03:15:18.647329Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e66ba0efc46d0f9831e4e65baa7d724638bc9b5b5de3f670e09858331aaedc73
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/4ZV2B36ENUHZQMPE4ZN2U7LSIY \
| 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: e66ba0efc46d0f9831e4e65baa7d724638bc9b5b5de3f670e09858331aaedc73
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "68f5a0e30099c8f4757af5de85f90949fe6e0c5049bbf6b092a12f50f0e7533a",
"cross_cats_sorted": [
"astro-ph.CO"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "gr-qc",
"submitted_at": "2012-10-15T17:03:39Z",
"title_canon_sha256": "3ec28749cbeaf4ffbb61695add7944c6e3e27cbe873793a89ebc7b4246fda046"
},
"schema_version": "1.0",
"source": {
"id": "1210.4106",
"kind": "arxiv",
"version": 2
}
}