Pith Number
pith:ATLNS26Y
pith:2018:ATLNS26YP322IKMSJUSLKUSTZE
not attested
not anchored
not stored
refs pending
Second-order cosmological perturbations. III. Produced by scalar-scalar coupling during radiation-dominated stage
arxiv:1811.06142 v3 · 2018-11-15 · gr-qc
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{ATLNS26YP322IKMSJUSLKUSTZE}
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 | 2026-05-17T23:54:53.412856Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
04d6d96bd87ef5a429924d24b55253c927b34bd73aa4f8d8ca8b7c4bb67e01bc
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/ATLNS26YP322IKMSJUSLKUSTZE \
| 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: 04d6d96bd87ef5a429924d24b55253c927b34bd73aa4f8d8ca8b7c4bb67e01bc
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a0fe7cffe69528ef01c3505a3b7e5568d8b64a26442170d4ad58457160c2d774",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "gr-qc",
"submitted_at": "2018-11-15T02:19:46Z",
"title_canon_sha256": "800ea9dae5f4c40b427516d04d6a6b2c811359bf3476cf8e4fdaf1d58d510328"
},
"schema_version": "1.0",
"source": {
"id": "1811.06142",
"kind": "arxiv",
"version": 3
}
}