Pith Number
pith:EVY2VAHM
pith:1997:EVY2VAHM7NTG4REEYV5HHBNSBS
not attested
not anchored
not stored
refs pending
Cosmological Perturbation Theory and the Spherical Collapse Model - I. Gaussian Initial Conditions
arxiv:astro-ph/9712095 v5 · 1997-12-05 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{EVY2VAHM7NTG4REEYV5HHBNSBS}
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.
Cited by
Receipt and verification
| First computed | 2026-07-04T16:03:31.290801Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
2571aa80ecfb666e4484c57a7385b20c851f18a7609c6fa520f762863a6ba797
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/EVY2VAHM7NTG4REEYV5HHBNSBS \
| 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: 2571aa80ecfb666e4484c57a7385b20c851f18a7609c6fa520f762863a6ba797
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "6fc712e8e82bf68b78b2f024ea3e0d1fcf18363f0bcc0f84dc28c0f9fd342372",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "1997-12-05T20:41:58Z",
"title_canon_sha256": "b89043b7e631f531e4bbfa58107811d4e1ac2a017ffbc39c84b175e2d13d959a"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/9712095",
"kind": "arxiv",
"version": 5
}
}