{
  "annotation_id": "c6ae6c4f-2994-434c-8616-46eaab617790",
  "date_created": "2026-03-02T18:00:46.595000Z",
  "date_modified": "2026-03-02T18:00:46.595000Z",
  "file_hash": "90908a6724194b4481c3262f3f44c56050e3751a4e7b1594144effe34625085f",
  "private": false,
  "record": {
    "abstract": "We suggest a new adiabatic approach for description of three charged\nparticles in the continuum. This approach is based on the Coulomb-Fourier\ntransformation (CFT) of three body Hamiltonian, which allows to develop a\nscheme, alternative to Born-Oppenheimer one.\n  The approach appears as an expansion of the kernels of corresponding integral\ntransformations in terms of small mass-ratio parameter. To be specific, the\nresults are presented for the system $ppe$ in the continuum. The wave function\nof a such system is compared with that one which is used for estimation of the\nrate for triple reaction $ p+p+e\\to d+\\nu, $ which take place as a step of\n$pp$-cycle in the center of the Sun. The problem of microscopic screening for\nthis particular reaction is discussed.",
    "arxiv_id": "physics/0310105",
    "authors": [
      "V. B. Belyaev",
      "S. B. Levin",
      "S. L. Yakovlev"
    ],
    "categories": [
      "physics.atom-ph",
      "physics.plasm-ph"
    ],
    "doi": "10.1088/0953-4075/37/6/018",
    "title": "Three charged particles in the continuum. Astrophysical examples",
    "url": "https://arxiv.org/abs/physics/0310105"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "6f4eabf6-a8c0-42ab-b5ea-c57bc3cee652",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}