Pith Number
pith:2RUV43EY
pith:2006:2RUV43EY4ZYMHL2HDXCWQBQAA3
not attested
not anchored
not stored
refs pending
Gravitational collapse of magnetized clouds. I. Ideal MHD accretion flow
arxiv:astro-ph/0604573 v1 · 2006-04-27 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{2RUV43EY4ZYMHL2HDXCWQBQAA3}
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 | 2026-07-04T15:19:43.248752Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d4695e6c98e670c3af471dc568060006ec7de24bd3c675812856ee2d10965658
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/2RUV43EY4ZYMHL2HDXCWQBQAA3 \
| 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: d4695e6c98e670c3af471dc568060006ec7de24bd3c675812856ee2d10965658
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "5040f7c807e0ab1b466d6310a7142e08b69a66902dc8db623f35914bfc9663e4",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2006-04-27T15:31:45Z",
"title_canon_sha256": "cf04d3d60794f902f40f1f0da26198549f7658fa246eeb51ef64cc55272a5a1f"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0604573",
"kind": "arxiv",
"version": 1
}
}