Pith Number
pith:HJ7JLZOU
pith:2018:HJ7JLZOUU7R2CEATZC4BLBQ3U5
not attested
not anchored
not stored
refs pending
Can generalized TOV equations explain neutron star macroscopic properties?
arxiv:1811.06445 v2 · 2018-11-15 · nucl-th
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{HJ7JLZOUU7R2CEATZC4BLBQ3U5}
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.
Receipt and verification
| First computed | 2026-05-17T23:52:39.854680Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3a7e95e5d4a7e3a11013c8b815861ba74ef4f67c7b52a12e31df1e2a0384591f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/HJ7JLZOUU7R2CEATZC4BLBQ3U5 \
| 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: 3a7e95e5d4a7e3a11013c8b815861ba74ef4f67c7b52a12e31df1e2a0384591f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2b95138f1f0b2d28cdb4e074637bbfdb829fb062d9fabe2856f0e68f5ee2bd85",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "nucl-th",
"submitted_at": "2018-11-15T16:04:18Z",
"title_canon_sha256": "4fe064cf34879b9ada4f1661c1186df2b2c6b1e558803d52b199778ea1b265aa"
},
"schema_version": "1.0",
"source": {
"id": "1811.06445",
"kind": "arxiv",
"version": 2
}
}