Pith Number
pith:H4PE7VSP
pith:2011:H4PE7VSPNZANYXH7IKZGFHTWHZ
not attested
not anchored
not stored
refs pending
Possibility of conversion of neutron star to quark star in presence of high magnetic field
arxiv:1102.4660 v2 · 2011-02-23 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{H4PE7VSPNZANYXH7IKZGFHTWHZ}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more
Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
Author claim
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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 | 2026-05-18T03:49:58.581883Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3f1e4fd64f6e40dc5cff42b2629e763e51631d94c8d6af77f49510d852a183c8
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/H4PE7VSPNZANYXH7IKZGFHTWHZ \
| 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: 3f1e4fd64f6e40dc5cff42b2629e763e51631d94c8d6af77f49510d852a183c8
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "ffb4bbd052ab2548471ab0e43d512f682c914cc59f038007bb6d40163a681818",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2011-02-23T04:50:56Z",
"title_canon_sha256": "4fd12b39eae79add3e75f83a75ed976392356d9f19558520b643e4c1b58fb0af"
},
"schema_version": "1.0",
"source": {
"id": "1102.4660",
"kind": "arxiv",
"version": 2
}
}