Pith Number
pith:WDID7TFR
pith:2002:WDID7TFRMTU7LLQJ7DG7GRXGNQ
not attested
not anchored
not stored
refs pending
The r-mode instability of neutron stars with the superfluid core
arxiv:astro-ph/0207415 v2 · 2002-07-19 · astro-ph · gr-qc
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{WDID7TFRMTU7LLQJ7DG7GRXGNQ}
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.
Receipt and verification
| First computed | 2026-07-04T14:12:07.250674Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b0d03fccb164e9f5ae09f8cdf346e66c21455e99cf75ce753709ecf8ee58175c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/WDID7TFRMTU7LLQJ7DG7GRXGNQ \
| 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: b0d03fccb164e9f5ae09f8cdf346e66c21455e99cf75ce753709ecf8ee58175c
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "38a69cd1bb7c4b044569040d6adb03e215c22d352d57a1863099b85b20839b12",
"cross_cats_sorted": [
"gr-qc"
],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2002-07-19T07:35:59Z",
"title_canon_sha256": "8aeb87119d966051fee3cba00e5d51b11ac3eedc3708741c9e6fafc41235f429"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0207415",
"kind": "arxiv",
"version": 2
}
}