{
  "annotation_id": "b8fcece9-a649-4647-9f58-3cc7a251951b",
  "date_created": "2026-03-02T18:00:07.973000Z",
  "date_modified": "2026-03-02T18:00:07.973000Z",
  "file_hash": "427d84893fb00c4a40bc7307843273e6982a8694c10890c690244f3e116f2f9c",
  "private": false,
  "record": {
    "abstract": "Beside its intrinsic interest for the insights it can give into color\nconfinement, knowledge of the space-time evolution of hadronization is very\nimportant for correctly interpreting jet-quenching data in heavy ion collisions\nand extracting the properties of the produced medium. On the experimental side,\nthe cleanest environment to study the space-time evolution of hadronization is\nsemi-inclusive Deeply Inelastic Scattering on nuclear targets. On the\ntheoretical side, 2 frameworks are presently competing to explain the observed\nattenuation of hadron production: quark energy loss (with hadron formation\noutside the nucleus) and nuclear absorption (with hadronization starting inside\nthe nucleus). I discuss recent observables and ideas which will help to\ndistinguish these 2 mechanisms and to measure the time scales of the\nhadronization process.",
    "arxiv_id": "nucl-th/0609010",
    "authors": [
      "Alberto Accardi"
    ],
    "categories": [
      "nucl-th",
      "hep-ph",
      "nucl-ex"
    ],
    "doi": "10.1140/epjc/s10052-006-0055-z",
    "journal_ref": "Eur.Phys.J.C49:347-353,2007",
    "title": "Space-time evolution of hadronization",
    "url": "https://arxiv.org/abs/nucl-th/0609010"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "7f440bc0-323d-4666-bc5b-75b74546783f",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}