Pith Number

pith:B2W2PZQK

pith:2018:B2W2PZQKEYDTFFDSWFYNGUHW3C

not attested not anchored not stored refs pending

Effects of a strong magnetic field on internal gravity waves: trapping, phase mixing, reflection and dynamical chaos

John C. B. Papaloizou, Shyeh Tjing Loi

arxiv:1804.03664 v1 · 2018-04-10 · astro-ph.SR · 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{B2W2PZQKEYDTFFDSWFYNGUHW3C}

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

Asteroseismology of solar-type stars

Receipt and verification

First computed	2026-05-18T00:17:37.818951Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

0eada7e60a2607329472b170d350f6d8b5b5ea47292e06efbd330727a45e096f

Aliases

arxiv: 1804.03664 · arxiv_version: 1804.03664v1 · doi: 10.48550/arxiv.1804.03664 · pith_short_12: B2W2PZQKEYDT · pith_short_16: B2W2PZQKEYDTFFDS · pith_short_8: B2W2PZQK

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/B2W2PZQKEYDTFFDSWFYNGUHW3C \
  | 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: 0eada7e60a2607329472b170d350f6d8b5b5ea47292e06efbd330727a45e096f

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "c318d6281d3f06b6cba6e7b1a543af88f52ee7093eb92bd2f842bc2bac5cc3c2",
    "cross_cats_sorted": [
      "physics.flu-dyn"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.SR",
    "submitted_at": "2018-04-10T18:00:07Z",
    "title_canon_sha256": "561efa94a58ad3bc9f9c2ca6db5b7baa9a04e14d4e2975f6949e2ad4c06b5def"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1804.03664",
    "kind": "arxiv",
    "version": 1
  }
}