{
  "annotation_id": "4dcf770f-0f36-48bb-9d9f-e01648b6e836",
  "date_created": "2026-03-02T18:01:10.854000Z",
  "date_modified": "2026-03-02T18:01:10.854000Z",
  "file_hash": "eb6a15c9ba207893ba02bf960d696918138f364b1bfca2699c7060201f2397a1",
  "private": false,
  "record": {
    "abstract": "An increasing number of numerical simulations and experiments describing the\nturbulent spectrum of Rayleigh-Taylor (RT) mixing layers came to light over the\npast few years. Results reported in recent studies allow to rule out a\nturbulence {\\it \\`a la Kolmogorov} as a mechanism acting on a self similar RT\nturbulent mixing layer. A different mechanism is presented, which complies with\nboth numerical and experimental results and relates RT flow to other buoyant\nflows.",
    "arxiv_id": "physics/0606136",
    "authors": [
      "Olivier Poujade"
    ],
    "categories": [
      "physics.plasm-ph",
      "astro-ph",
      "physics.flu-dyn"
    ],
    "doi": "10.1103/PhysRevLett.97.185002",
    "journal_ref": "Phys.Rev.Lett. 97 (2006) 185002",
    "title": "Rayleigh-Taylor turbulence is nothing like Kolmogorov turbulence in the   self similar regime",
    "url": "https://arxiv.org/abs/physics/0606136"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "3215e2f0-2b3b-4801-81fe-707743d15202",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}