Pith Number
pith:O6T5C6ZM
pith:2017:O6T5C6ZMLLJQJT52N6N4CM4G53
not attested
not anchored
not stored
refs pending
Supercritical Accretion onto a Non-Magnetized Neutron Star: Why is it Feasible?
arxiv:1712.02068 v1 · 2017-12-06 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{O6T5C6ZMLLJQJT52N6N4CM4G53}
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 | 2026-05-18T00:24:14.984565Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
77a7d17b2c5ad304cfba6f9bc13386eee8db4b888c97bac76c0ea6c06f5a1840
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/O6T5C6ZMLLJQJT52N6N4CM4G53 \
| 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: 77a7d17b2c5ad304cfba6f9bc13386eee8db4b888c97bac76c0ea6c06f5a1840
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "cc4b5b5960cceb6e70174474d2a46a042ab06177f7cf5a1777d5185a5e167f38",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2017-12-06T07:47:51Z",
"title_canon_sha256": "5bad9574ca663b7dbd1982490eef3586a039fa591d28a6b1ad184b9f344558f4"
},
"schema_version": "1.0",
"source": {
"id": "1712.02068",
"kind": "arxiv",
"version": 1
}
}