Pith Number
pith:K62Z352O
pith:2023:K62Z352OWC7DHXCGYKCI6GH5CR
not attested
not anchored
not stored
refs pending
Which first order phase transitions to quark matter are possible in neutron stars?
arxiv:2312.10148 v2 · 2023-12-15 · nucl-th · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{K62Z352OWC7DHXCGYKCI6GH5CR}
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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 | 2026-07-05T07:59:59.019676Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
57b59df74eb0be33dc46c2848f18fd1450e0be8e1841a19306aa1ffeeacf7b40
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/K62Z352OWC7DHXCGYKCI6GH5CR \
| 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: 57b59df74eb0be33dc46c2848f18fd1450e0be8e1841a19306aa1ffeeacf7b40
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "5e704a7e3efbcf513929b65520fa6ef3eadf176584741c4013e25fce09cabdf0",
"cross_cats_sorted": [
"astro-ph.HE"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "nucl-th",
"submitted_at": "2023-12-15T19:00:26Z",
"title_canon_sha256": "6a351994cd2c5aae58259486e4bb24ebcbc90d644467759dc4c1dd362895759b"
},
"schema_version": "1.0",
"source": {
"id": "2312.10148",
"kind": "arxiv",
"version": 2
}
}