Pith Number
pith:HKPQP4OI
pith:2017:HKPQP4OIXZDGAT23YSTZ3RVIWR
not attested
not anchored
not stored
refs pending
Plunging neutron stars as origin of organised magnetic field in galactic nuclei
arxiv:1705.09820 v1 · 2017-05-27 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{HKPQP4OIXZDGAT23YSTZ3RVIWR}
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 | 2026-05-18T00:37:41.943649Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3a9f07f1c8be46604f5bc4a79dc6a8b4612ac21e4179eee5e3a4f3938febf453
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/HKPQP4OIXZDGAT23YSTZ3RVIWR \
| 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: 3a9f07f1c8be46604f5bc4a79dc6a8b4612ac21e4179eee5e3a4f3938febf453
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3a4276f37750bcd70888dc9791b6e5e0f23d3d27bd7e11f4a9d5af613929b5ff",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2017-05-27T14:08:51Z",
"title_canon_sha256": "d29906bf01edac0d9d5b75d379f3dd6482b2358963ea158fe104fc90067af4d3"
},
"schema_version": "1.0",
"source": {
"id": "1705.09820",
"kind": "arxiv",
"version": 1
}
}