Pith Number

pith:BL75JZA6

pith:2017:BL75JZA6JYNHOQS5V3Q4JVU2WW

not attested not anchored not stored refs pending

The dynamo effect in decaying helical turbulence

Alberto Roper Pol, Alexander G. Tevzadze, Axel Brandenburg, Sayan Mandal, Tanmay Vachaspati, Tina Kahniashvili

arxiv:1710.01628 v4 · 2017-10-04 · physics.flu-dyn · astro-ph.CO

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

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{BL75JZA6JYNHOQS5V3Q4JVU2WW}

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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

2 papers in Pith

Primordial black holes and magnetic fields in conformal neutrino mass models

Primordial Magnetogenesis and Gravitational Waves from ALP-assisted Phase Transition

Receipt and verification

First computed	2026-05-17T23:52:44.471728Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

0affd4e41e4e1a77425daee1c4d69ab59a2094960db8d612d007119bdb6e27c1

Aliases

arxiv: 1710.01628 · arxiv_version: 1710.01628v4 · doi: 10.48550/arxiv.1710.01628 · pith_short_12: BL75JZA6JYNH · pith_short_16: BL75JZA6JYNHOQS5 · pith_short_8: BL75JZA6

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/BL75JZA6JYNHOQS5V3Q4JVU2WW \
  | 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: 0affd4e41e4e1a77425daee1c4d69ab59a2094960db8d612d007119bdb6e27c1

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "5988f1a87a48b7f8d605175cf408c00545c6741c636793b47630f5182a31eef5",
    "cross_cats_sorted": [
      "astro-ph.CO"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "physics.flu-dyn",
    "submitted_at": "2017-10-04T14:43:44Z",
    "title_canon_sha256": "f2998fa3f8118d1e8d5214e36e30eb167543763c995219a7ecb233ea7f13e6b4"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1710.01628",
    "kind": "arxiv",
    "version": 4
  }
}