Pith Number
pith:CW3DDTSO
pith:2013:CW3DDTSOVHV3P7RY25UEVEV7QP
not attested
not anchored
not stored
refs pending
Does a hadron-quark phase transition in dense matter preclude the existence of massive neutron stars ?
arxiv:1304.6907 v1 · 2013-04-25 · astro-ph.HE · nucl-th
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{CW3DDTSOVHV3P7RY25UEVEV7QP}
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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.
Receipt and verification
| First computed | 2026-05-18T03:27:10.811637Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
15b631ce4ea9ebb7fe38d7684a92bf83c8d1a29858e46975862ff1c7cf6a67c7
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/CW3DDTSOVHV3P7RY25UEVEV7QP \
| 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: 15b631ce4ea9ebb7fe38d7684a92bf83c8d1a29858e46975862ff1c7cf6a67c7
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "32a84ec0381329f7de41b1993dad3f1c0e1158c576732a20561f270db7130f56",
"cross_cats_sorted": [
"nucl-th"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2013-04-25T13:48:15Z",
"title_canon_sha256": "8d3c096b30f3e55574e5e7a4ae2268c163e83d359a88c8b0bc05051c6fba6e2b"
},
"schema_version": "1.0",
"source": {
"id": "1304.6907",
"kind": "arxiv",
"version": 1
}
}