Pith Number
pith:HWYEMDNJ
pith:2021:HWYEMDNJP4VTIDG2GJT6VQPC6O
not attested
not anchored
not stored
refs pending
Stability of Neutron Stars with Dark Matter Core Using Three Crustal Types and the Impact on Mass-Radius Relations
arxiv:2104.04969 v2 · 2021-04-11 · nucl-th
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{HWYEMDNJP4VTIDG2GJT6VQPC6O}
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 | 2026-07-05T05:43:45.359135Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3db0460da97f2b340cda3267eac1e2f38b4fcfa6bce413644ae75ae02f45448f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/HWYEMDNJP4VTIDG2GJT6VQPC6O \
| 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: 3db0460da97f2b340cda3267eac1e2f38b4fcfa6bce413644ae75ae02f45448f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "cce1268ed08430a0d6e9286ece9214f09818200aaa145aed42288ec01df11cec",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "nucl-th",
"submitted_at": "2021-04-11T09:22:23Z",
"title_canon_sha256": "f139328a1ccd9e01d55dc1b19398faf1473b112eda9679a36671c67d6e80e69e"
},
"schema_version": "1.0",
"source": {
"id": "2104.04969",
"kind": "arxiv",
"version": 2
}
}