Pith Number
pith:3YVZLFD5
pith:2011:3YVZLFD5RVAW2HS6A5S4NUM4GJ
not attested
not anchored
not stored
refs pending
WMAP7 and future CMB constraints on annihilating dark matter: implications for GeV-scale WIMPs
arxiv:1103.2766 v3 · 2011-03-14 · astro-ph.CO · hep-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{3YVZLFD5RVAW2HS6A5S4NUM4GJ}
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.
Cited by
Receipt and verification
| First computed | 2026-05-18T02:02:53.602961Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
de2b95947d8d416d1e5e0765c6d19c326a191f986f477b394ea92caeb804e81b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/3YVZLFD5RVAW2HS6A5S4NUM4GJ \
| 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: de2b95947d8d416d1e5e0765c6d19c326a191f986f477b394ea92caeb804e81b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "20e7d86f8c33e0ec20416667d18bc3411093bff9e253f38fada7503a83970db1",
"cross_cats_sorted": [
"hep-ph"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2011-03-14T19:59:49Z",
"title_canon_sha256": "69116c9cad4014c2173a2a88470fcd92068414bbfdbbfaa6a5ae0be9206d908a"
},
"schema_version": "1.0",
"source": {
"id": "1103.2766",
"kind": "arxiv",
"version": 3
}
}