Pith Number
pith:BHYTZSHZ
pith:1998:BHYTZSHZH44XMNK3AXLFUHZSYU
not attested
not anchored
not stored
refs pending
Which fraction of the measured cosmic-ray antiprotons might be due to neutralino annihilation in the galactic halo?
arxiv:astro-ph/9804137 v1 · 1998-04-14 · astro-ph · hep-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{BHYTZSHZH44XMNK3AXLFUHZSYU}
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.
Receipt and verification
| First computed | 2026-05-18T04:34:28.998126Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
09f13cc8f93f3976355b05d65a1f32c533a0a70503d014bbdb40e7036be57a68
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/BHYTZSHZH44XMNK3AXLFUHZSYU \
| 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: 09f13cc8f93f3976355b05d65a1f32c533a0a70503d014bbdb40e7036be57a68
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "30edbbcfb7fb45e4202058bcd7b0fbcb0dcf15a9d62a463e1103d2c0552b1f3c",
"cross_cats_sorted": [
"hep-ph"
],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "1998-04-14T18:21:58Z",
"title_canon_sha256": "af48a7fa741f90c4b1b3f95c0cff6506fbbcea3d445e678b7d8f2c7d3f541198"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/9804137",
"kind": "arxiv",
"version": 1
}
}