{
  "annotation_id": "3c1a07c7-42ca-4fab-b07f-7d02cdf64199",
  "date_created": "2026-03-02T18:00:19.110000Z",
  "date_modified": "2026-03-02T18:00:19.110000Z",
  "file_hash": "f1b3ff00f979330d92d1cf3b6f8194976e1475a6512a9650cb49af808b50796f",
  "private": false,
  "record": {
    "abstract": "Using a (3+1)-dimensional solution of the relativistic Euler-equations for\n$Pb+Pb$ at 160 $AGeV$, space-time extensions of kaon emission zones are\ncalculated from space-time densities and compared to the inverse widths of\ntwo-kaon Bose-Einstein correlation functions. The comparison shows a\nsatisfactory agreement and it is concluded that because of the Gaussian shape\nof the kaon correlation functions, the space-time parameters of the kaon source\ncan be calculated directly from space-time densities. In the case of intensity\ninterferometry of identical pions this simplification is not recommended when\napplying Gaussian fits because of the present strong effects of resonance\ndecays. The whole discussion is based on the assumption that hadron emission in\nultra-relativistic heavy-ion collisions is purely chaotic or that coherence is\nat least negligible.",
    "arxiv_id": "nucl-th/9605016",
    "authors": [
      "B. R. Schlei"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.55.954",
    "journal_ref": "Phys.Rev.C55:954-957,1997",
    "title": "Space-time extensions from space-time densities and Bose-Einstein   correlations",
    "url": "https://arxiv.org/abs/nucl-th/9605016"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "f474b198-cc0f-40bd-8052-d77c4e71a412",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}