Pith Number
pith:V5V2C3RG
pith:2018:V5V2C3RGHMTLV727MSVXWUQPQZ
not attested
not anchored
not stored
refs pending
Temperature-dependent oscillation modes in rotating superfluid neutron stars
arxiv:1810.08005 v1 · 2018-10-18 · astro-ph.HE · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{V5V2C3RGHMTLV727MSVXWUQPQZ}
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 | 2026-05-18T00:01:26.074803Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
af6ba16e263b26baff5f64ab7b520f864d3cca155aed8ad3448deac46b106c10
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/V5V2C3RGHMTLV727MSVXWUQPQZ \
| 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: af6ba16e263b26baff5f64ab7b520f864d3cca155aed8ad3448deac46b106c10
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "5ddf7455b009f65e6a8a44c50fbd444ebd46a6366da66bb1e06eee7a3de2e6f1",
"cross_cats_sorted": [
"astro-ph.SR"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2018-10-18T12:07:53Z",
"title_canon_sha256": "2f343ea5b1eed711ffe91dc78db93a1e6faca169f934d3ce2adad560a2e47c61"
},
"schema_version": "1.0",
"source": {
"id": "1810.08005",
"kind": "arxiv",
"version": 1
}
}