Pith Number
pith:HKS4NYWF
pith:2010:HKS4NYWF6LEKA7HXLHE3ZHYP5E
not attested
not anchored
not stored
refs pending
Can eccentric binary millisecond pulsars form by accretion induced collapse of white dwarfs?
arxiv:1008.2130 v2 · 2010-08-12 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{HKS4NYWF6LEKA7HXLHE3ZHYP5E}
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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.
Receipt and verification
| First computed | 2026-05-18T02:05:49.001293Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3aa5c6e2c5f2c8a07cf759c9bc9f0fe9183811b3f965cfc90820c319802efbef
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/HKS4NYWF6LEKA7HXLHE3ZHYP5E \
| 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: 3aa5c6e2c5f2c8a07cf759c9bc9f0fe9183811b3f965cfc90820c319802efbef
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3ac28c50216ea284fe695b93b8b52edf30a5bcb22545bb6db20672c09bc98f00",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2010-08-12T15:11:39Z",
"title_canon_sha256": "2db3b9e72a11b2dbc478fa2e6bcf8425e3958a5e3d35356a6aa514b66c225ba8"
},
"schema_version": "1.0",
"source": {
"id": "1008.2130",
"kind": "arxiv",
"version": 2
}
}