Pith Number

pith:QCHWLJZ4

pith:2026:QCHWLJZ423RUAAQMT66NHPRHGT

not attested not anchored not stored refs pending

On The Nonthermal Power Laws In Magnetized Turbulent Plasmas

Alexander Philippov, Daniel Gro\v{s}elj, Rostom Mbarek

A scaling law derived from particle transport predicts nonthermal spectral tails in magnetized turbulent plasmas.

arxiv:2605.03033 v2 · 2026-05-04 · physics.plasm-ph · astro-ph.HE

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\pithnumber{QCHWLJZ423RUAAQMT66NHPRHGT}

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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.

Claims

C1strongest claim

We derive a scaling law for the formation of nonthermal spectral tails in mildly and strongly magnetized turbulent environments. The simulation results show good agreement with our theoretical predictions.

C2weakest assumption

The scaling law rests on assumptions from recent progress in particle transport in magnetized plasmas; the precise transport model and the conditions under which the scaling applies are not detailed in the abstract.

C3one line summary

A scaling law for nonthermal power-law tails in magnetized turbulent plasmas is derived from particle transport principles and confirmed by PIC simulations with escape, with applications to black hole coronae.

Cited by

1 paper in Pith

Particle Acceleration, Coronal Neutrino Production, and the Diffuse Extragalactic Neutrino Background from Supermassive Black Holes

Receipt and verification

First computed	2026-05-28T02:04:48.911742Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

808f65a73cd6e340020c9fbcd3be2734d01288dcd2841e8e0b224007ce0b9ab8

Aliases

arxiv: 2605.03033 · arxiv_version: 2605.03033v2 · doi: 10.48550/arxiv.2605.03033 · pith_short_12: QCHWLJZ423RU · pith_short_16: QCHWLJZ423RUAAQM · pith_short_8: QCHWLJZ4

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Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/QCHWLJZ423RUAAQMT66NHPRHGT \
  | 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: 808f65a73cd6e340020c9fbcd3be2734d01288dcd2841e8e0b224007ce0b9ab8

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "91cde978c81eb67db871a6a0b202793817a4684a91a58ac5e11ebc79b9f3ed48",
    "cross_cats_sorted": [
      "astro-ph.HE"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "physics.plasm-ph",
    "submitted_at": "2026-05-04T18:02:14Z",
    "title_canon_sha256": "d4b9db441cc68a821efbeb02ab509172f15a6f9c74d2948e9ccab9fb78a9a275"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.03033",
    "kind": "arxiv",
    "version": 2
  }
}