Pith Number
pith:A23RF26E
pith:2023:A23RF26EIYBUB2CX4LECNSXIGO
not attested
not anchored
not stored
refs pending
Can prompt cusps of WIMP dark matter be detected as individual gamma-ray sources?
arxiv:2310.15214 v2 · 2023-10-23 · astro-ph.CO · astro-ph.HE · hep-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{A23RF26EIYBUB2CX4LECNSXIGO}
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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
Detecting dark matter sub-halos in the Galactic plane with the Cherenkov Telescope Array Observatory
Receipt and verification
| First computed | 2026-07-05T07:39:31.249292Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
06b712ebc4460340e857e2c826cae833ba490dc6750e0d0c78d9ba4393d8218b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/A23RF26EIYBUB2CX4LECNSXIGO \
| 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: 06b712ebc4460340e857e2c826cae833ba490dc6750e0d0c78d9ba4393d8218b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a78e5e4dce46bdbe27e6e72d1d9f188a8d22b87e8dc319dd144551820d9c6eb7",
"cross_cats_sorted": [
"astro-ph.HE",
"hep-ph"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2023-10-23T18:00:00Z",
"title_canon_sha256": "c463377ea8d903be55edd5696fe56951465a97487900cb887f754b1c5ad64f29"
},
"schema_version": "1.0",
"source": {
"id": "2310.15214",
"kind": "arxiv",
"version": 2
}
}