Pith Number
pith:C65QD6U6
pith:2024:C65QD6U64SG6FLYZR5LA5PJ7FQ
not attested
not anchored
not stored
refs pending
Scalar emission from neutron star-black hole binaries in scalar-tensor theories with kinetic screening
arxiv:2410.16367 v1 · 2024-10-21 · gr-qc
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{C65QD6U64SG6FLYZR5LA5PJ7FQ}
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 | 2026-07-05T10:59:25.347629Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
17bb01fa9ee48de2af198f560ebd3f2c27f437973293c9aaecdc73343b514ef0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/C65QD6U64SG6FLYZR5LA5PJ7FQ \
| 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: 17bb01fa9ee48de2af198f560ebd3f2c27f437973293c9aaecdc73343b514ef0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "7a3fdcb7ec0f481b4f38254214fe9bf2523ffa1382a5229d0f11500b21e8cc7e",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "gr-qc",
"submitted_at": "2024-10-21T18:00:02Z",
"title_canon_sha256": "2ca939398948a70855f776e62372e1f83c7fba64f774b3567f8ddada22d61d24"
},
"schema_version": "1.0",
"source": {
"id": "2410.16367",
"kind": "arxiv",
"version": 1
}
}