Pith Number
pith:J4MVF62H
pith:2006:J4MVF62HY3D5NRYXWKFGHTP6FY
not attested
not anchored
not stored
refs pending
Formation and Collapse of Nonaxisymmetric Protostellar Cores in Planar Magnetic Interstellar Clouds: Formulation of the Problem and Linear Analysis
arxiv:astro-ph/0607622 v1 · 2006-07-27 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{J4MVF62HY3D5NRYXWKFGHTP6FY}
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 | 2026-05-18T04:28:58.211018Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
4f1952fb47c6c7d6c717b28a63cdfe2e220a917bfe959ee31a6583bb9de41e2c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/J4MVF62HY3D5NRYXWKFGHTP6FY \
| 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: 4f1952fb47c6c7d6c717b28a63cdfe2e220a917bfe959ee31a6583bb9de41e2c
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "0fb7da815b837433a360585afeb930548601d89c3359340e4ae3e86e45568c91",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2006-07-27T18:27:31Z",
"title_canon_sha256": "20ab8c545e314e25af3e2c4d2ac7a42d2f46729d02840754bba1a0019d4f1b39"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0607622",
"kind": "arxiv",
"version": 1
}
}