Pith Number
pith:KZWEBXLL
pith:2015:KZWEBXLLIV6PWSERQTP4643NI3
not attested
not anchored
not stored
refs pending
Are dark energy models with variable EoS parameter $w$ compatible with the late inhomogeneous Universe?
arxiv:1502.04693 v2 · 2015-02-16 · gr-qc · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{KZWEBXLLIV6PWSERQTP4643NI3}
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 | 2026-05-18T01:36:25.706991Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
566c40dd6b457cfb489184dfcf736d46f1c0c239465076ef1dfd19e5a097c300
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KZWEBXLLIV6PWSERQTP4643NI3 \
| 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: 566c40dd6b457cfb489184dfcf736d46f1c0c239465076ef1dfd19e5a097c300
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "c34f0256326d7e70a7216a59f54bce4d0d64acd5ab6e54d6aedb9573212e00bf",
"cross_cats_sorted": [
"astro-ph.CO"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "gr-qc",
"submitted_at": "2015-02-16T20:56:55Z",
"title_canon_sha256": "32a78a86b597f93b991582b9522daff40dcacad9db8dc078bc6c818a9de028dd"
},
"schema_version": "1.0",
"source": {
"id": "1502.04693",
"kind": "arxiv",
"version": 2
}
}