Pith Number
pith:2HH3XNMG
pith:2025:2HH3XNMGI4VYY5PTA7ZN7TTWZB
not attested
not anchored
not stored
refs pending
Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: I. Survey of Eddington Ratios
arxiv:2506.02289 v2 · 2025-06-02 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{2HH3XNMGI4VYY5PTA7ZN7TTWZB}
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.
Cited by
Receipt and verification
| First computed | 2026-07-05T12:11:18.493989Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d1cfbbb586472b8c75f307f2dfce76c87cc13adc2483efec8a0e02f942db4fa3
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/2HH3XNMGI4VYY5PTA7ZN7TTWZB \
| 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: d1cfbbb586472b8c75f307f2dfce76c87cc13adc2483efec8a0e02f942db4fa3
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "67d2e0a5840381f64bf57c6fdadb6abde4803046affce15a107d353cdc0409c3",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2025-06-02T21:59:09Z",
"title_canon_sha256": "6372edb83df30bd406daca47c6714e78636b0047d95952c8afa54107d51cc3d9"
},
"schema_version": "1.0",
"source": {
"id": "2506.02289",
"kind": "arxiv",
"version": 2
}
}