Pith Number
pith:GFNUHJCZ
pith:2024:GFNUHJCZA43GUKNC743FDBLE3R
not attested
not anchored
not stored
refs pending
Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension
arxiv:2404.15977 v3 · 2024-04-24 · gr-qc · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{GFNUHJCZA43GUKNC743FDBLE3R}
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
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-07-05T10:17:46.984446Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
315b43a45907366a29a2ff36518564dc7bd5c148e612c1b0ea5d838064807cac
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/GFNUHJCZA43GUKNC743FDBLE3R \
| 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: 315b43a45907366a29a2ff36518564dc7bd5c148e612c1b0ea5d838064807cac
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f95d42b8edfbba2e169735db0c2fdc2e72d3946a65cd66ec2c3ef0d25c5da2e5",
"cross_cats_sorted": [
"astro-ph.CO"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "gr-qc",
"submitted_at": "2024-04-24T16:52:15Z",
"title_canon_sha256": "c3a557ebfcc40d32f2e8bb0cabfdb65ef7d75363ebc23c3d32f37c9dbc2d98a8"
},
"schema_version": "1.0",
"source": {
"id": "2404.15977",
"kind": "arxiv",
"version": 3
}
}