Pith Number
pith:JZXKB6YY
pith:2024:JZXKB6YYY42B5YHKNYGFWKBIP7
not attested
not anchored
not stored
refs pending
Magnetic Flux Transport in Advection Dominated Accretion Flow Towards the Formation of Magnetically Arrested Disk
arxiv:2411.18258 v1 · 2024-11-27 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{JZXKB6YYY42B5YHKNYGFWKBIP7}
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 | 2026-07-05T09:41:13.930417Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
4e6ea0fb18c7341ee0ea6e0c5b28287fd75ed0c7de5ea48acac060f24208b414
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/JZXKB6YYY42B5YHKNYGFWKBIP7 \
| 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: 4e6ea0fb18c7341ee0ea6e0c5b28287fd75ed0c7de5ea48acac060f24208b414
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2576057f3f157ba4c268e6690f552ef5f8e10d1c4e5e412967a9af0735747a46",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2024-11-27T11:56:55Z",
"title_canon_sha256": "45efee27518806c8334974e6fc480a377dcea98ab5876cd31a5d4b2106a843d0"
},
"schema_version": "1.0",
"source": {
"id": "2411.18258",
"kind": "arxiv",
"version": 1
}
}