{
  "annotation_id": "8a6226c0-c4bb-4052-9087-39c576bd4e6b",
  "date_created": "2026-03-02T18:00:15.479000Z",
  "date_modified": "2026-03-02T18:00:15.479000Z",
  "file_hash": "617bede2a62322a69484aba86b1a6f0cd57dbc2dae758b62ef1145ad2bfe362b",
  "private": false,
  "record": {
    "abstract": "We re-examine the matter radii of diffuse halo nuclei, as deduced from\nreaction cross section measurements at high energy. Careful consideration is\ngiven to the intrinsic few-body structure of these projectiles and the\nadiabatic nature of the projectile-target interaction. Using $^{11}$Li,\n$^{11}$Be and $^{8}$B as examples we show that data require significantly\nlarger matter radii than previously reported. The revised value for $^{11}$Li\nof 3.55 fm is consistent with three-body models with significant $1s$-intruder\nstate components, which reproduce experimental $^{9}$Li momentum distributions\nfollowing $^{11}$Li breakup, but were hitherto thought to be at variance with\ncross section data.",
    "arxiv_id": "nucl-th/9604033",
    "authors": [
      "J. S. Al-Khalili",
      "J. A. Tostevin"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevLett.76.3903",
    "journal_ref": "Phys.Rev.Lett.76:3903-3906,1996",
    "title": "Matter radii of light halo nuclei",
    "url": "https://arxiv.org/abs/nucl-th/9604033"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "17eb7e27-203e-4242-bfe8-9931a0fd8cc3",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}