Pith Number
pith:4RNLNPLH
pith:2016:4RNLNPLH3UP4BN3MVIZD7R7QWS
not attested
not anchored
not stored
refs pending
Characteristic Properties of Two Different Viscous Cosmology Models for the Future Universe
arxiv:1612.01794 v1 · 2016-12-06 · gr-qc · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{4RNLNPLH3UP4BN3MVIZD7R7QWS}
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
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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 | 2026-05-18T00:52:54.901200Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e45ab6bd67dd1fc0b76caa323fc7f0b4b6d5f8e821a8cda2f0101ccb490957c5
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/4RNLNPLH3UP4BN3MVIZD7R7QWS \
| 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: e45ab6bd67dd1fc0b76caa323fc7f0b4b6d5f8e821a8cda2f0101ccb490957c5
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f83403724f71e0467830c49f1810035a2f67afdb287eb25ab16215c876697200",
"cross_cats_sorted": [
"astro-ph.CO"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "gr-qc",
"submitted_at": "2016-12-06T13:10:11Z",
"title_canon_sha256": "dc12b446c5dac15df7c314ba62bc5519dafc0c000bb1a5568be05451642591d9"
},
"schema_version": "1.0",
"source": {
"id": "1612.01794",
"kind": "arxiv",
"version": 1
}
}