Pith Number

pith:3XEVJGCP

pith:2001:3XEVJGCP7ZGLO3CQAYL4L2N3MP

not attested not anchored not stored refs pending

Kolmogorov-Burgers Model for Star Forming Turbulence

Santa Barbara), Stanislav Boldyrev (Institute for Theoretical Physics

arxiv:astro-ph/0108300 v2 · 2001-08-18 · astro-ph · cond-mat · nlin.CD · physics.flu-dyn

Open paper page JSON Open Graph Bundle Merged state Verified badge What is a Pith Number?

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{3XEVJGCP7ZGLO3CQAYL4L2N3MP}

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 open · sign in to claim

4 Citations open

5 Replications open

✓ 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

1 paper in Pith

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas

Receipt and verification

First computed	2026-07-04T16:23:59.232919Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

ddc954984ffe4cb76c500617c5e9bb63ee96fa9644ee678c790495825ee51d08

Aliases

arxiv: astro-ph/0108300 · arxiv_version: astro-ph/0108300v2 · doi: 10.48550/arxiv.astro-ph/0108300 · pith_short_12: 3XEVJGCP7ZGL · pith_short_16: 3XEVJGCP7ZGLO3CQ · pith_short_8: 3XEVJGCP

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/3XEVJGCP7ZGLO3CQAYL4L2N3MP \
  | 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: ddc954984ffe4cb76c500617c5e9bb63ee96fa9644ee678c790495825ee51d08

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "ac354307ff6f46798122e177798a1bbfb7b683797b0d3aee0d121861adeb3b33",
    "cross_cats_sorted": [
      "cond-mat",
      "nlin.CD",
      "physics.flu-dyn"
    ],
    "license": "",
    "primary_cat": "astro-ph",
    "submitted_at": "2001-08-18T01:56:14Z",
    "title_canon_sha256": "4d7c967cd628a8f39886df1a21b653fc5437dd9ca1b9491fdcbdf88bca42c16f"
  },
  "schema_version": "1.0",
  "source": {
    "id": "astro-ph/0108300",
    "kind": "arxiv",
    "version": 2
  }
}