{
  "annotation_id": "6d13da4f-0c35-459d-8c62-fd2255e2b90b",
  "date_created": "2026-03-02T18:00:10.884000Z",
  "date_modified": "2026-03-02T18:00:10.884000Z",
  "file_hash": "71d0e595839e26d0721372ac0b76f3e8bae5d14ee448523fbad78ec06a083987",
  "private": false,
  "record": {
    "abstract": "The semi-relativistic approach to electron and neutrino quasielastic\nscattering from nuclei is extended to include final-state interactions.\nStarting with the usual non-relativistic continuum shell model, the problem is\nrelativized by using the semi-relativistic expansion of the current in powers\nof the initial nucleon momentum and relativistic kinematics. Two different\napproaches are considered for the final-state interactions: the Smith-Wambach\n2p-2h damping model and the Dirac-equation-based potential extracted from a\nrelativistic mean-field plus the Darwin factor. Using the latter the scaling\nproperties of $(e,e\u0027)$ and $(\\nu_\\mu,\\mu^-)$ cross sections for intermediate\nmomentum transfers are investigated.",
    "arxiv_id": "nucl-th/0612056",
    "authors": [
      "J. E. Amaro",
      "M. B. Barbaro",
      "J. A. Caballero",
      "T. W. Donnelly",
      "J. M. Udias"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.75.034613",
    "journal_ref": "Phys.Rev.C75:034613,2007",
    "title": "Final-state interactions and superscaling in the semi-relativistic   approach to quasielastic electron and neutrino scattering",
    "url": "https://arxiv.org/abs/nucl-th/0612056"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "33025e50-f077-46dc-b223-5b9bbfb2c02e",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}