Pith Number
pith:D7IJLXAK
pith:2005:D7IJLXAKEB6E2NX3QNCKLDGHCD
not attested
not anchored
not stored
refs pending
Two-Dimensional Hydrodynamic Core-Collapse Supernova Simulations with Spectral Neutrino Transport II. Models for Different Progenitor Stars
arxiv:astro-ph/0512189 v2 · 2005-12-07 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{D7IJLXAKEB6E2NX3QNCKLDGHCD}
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 | 2026-07-04T16:53:08.096330Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
1fd095dc0a207c4d36fb8344a58cc710eac689a687dbd4f8eb9caa5225534dcf
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/D7IJLXAKEB6E2NX3QNCKLDGHCD \
| 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: 1fd095dc0a207c4d36fb8344a58cc710eac689a687dbd4f8eb9caa5225534dcf
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "0e006838b28c4cda7bb697f431d58c696a97ef90c4baaaa10aca283211a8f720",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2005-12-07T17:30:52Z",
"title_canon_sha256": "0aa8d01bd9ac8b3071bf46a99bea08f5dcc4cf2eefb80a4aa1c0fe445f62ad84"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0512189",
"kind": "arxiv",
"version": 2
}
}