Pith Number
pith:Q5X3OPZF
pith:2018:Q5X3OPZFJ5FZ5M36ZCWNRYOH3U
not attested
not anchored
not stored
refs pending
Plasma Perturbations and Cosmic Microwave Background Anisotropy in the Linearly Expanding Milne-like Universe
arxiv:1803.09094 v2 · 2018-03-24 · gr-qc · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{Q5X3OPZFJ5FZ5M36ZCWNRYOH3U}
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 | 2026-05-17T23:56:48.207470Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
876fb73f254f4b9eb37ec8acd8e1c7dd3d584189f5c61c10d166a85ef2f2e83b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/Q5X3OPZFJ5FZ5M36ZCWNRYOH3U \
| 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: 876fb73f254f4b9eb37ec8acd8e1c7dd3d584189f5c61c10d166a85ef2f2e83b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3dd6926994cd312869ab11343a3c7ec8b6e1f7bf1311a18b8565c37aed3a10c4",
"cross_cats_sorted": [
"astro-ph.CO"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "gr-qc",
"submitted_at": "2018-03-24T11:22:25Z",
"title_canon_sha256": "d1af36f34efa6ea3c5c2f33f356787d55d0b30299da84d96bd9cceb7c78de711"
},
"schema_version": "1.0",
"source": {
"id": "1803.09094",
"kind": "arxiv",
"version": 2
}
}