Pith Number
pith:S5PFWMLG
pith:2024:S5PFWMLGLDHRCO6UYC5ZWDCM3X
not attested
not anchored
not stored
refs pending
Dark Matter Influence on Quarkyonic Stars: A Relativistic Mean Field Analysis
arxiv:2401.02190 v2 · 2024-01-04 · astro-ph.HE · nucl-th
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{S5PFWMLGLDHRCO6UYC5ZWDCM3X}
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.
Cited by
Receipt and verification
| First computed | 2026-07-05T11:49:31.022384Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
975e5b316658cf113bd4c0bb9b0c4cddfcceaba403f3be7ecf41f8e4f5cadc81
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/S5PFWMLGLDHRCO6UYC5ZWDCM3X \
| 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: 975e5b316658cf113bd4c0bb9b0c4cddfcceaba403f3be7ecf41f8e4f5cadc81
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "372fa2f24a28ff3f725466097a9a758190304932c1012b282a16c0f7991e0486",
"cross_cats_sorted": [
"nucl-th"
],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2024-01-04T10:43:02Z",
"title_canon_sha256": "2618cbeca519b7496a80ffb7bd3edf8a32ebbb1e3b6b98416de6e608623a2dec"
},
"schema_version": "1.0",
"source": {
"id": "2401.02190",
"kind": "arxiv",
"version": 2
}
}