{
  "annotation_id": "135b6315-a4a1-4d3b-acf7-850b08da339f",
  "date_created": "2026-03-02T18:00:46.977000Z",
  "date_modified": "2026-03-02T18:00:46.977000Z",
  "file_hash": "f5daa6acc1e4d90aad6a71eaa5992a91e0cf8f00d1f36f5e7a23267b2c1ba83f",
  "private": false,
  "record": {
    "abstract": "The studies realized in INRNE (Institute for Nuclear Research and Nuclear\nEnergy) particulary in cosmic rays detection and construction of Muonic\nCerenkov Telescope in University of Blagoevgrad [1] shows the need to develop a\ntheoretical model based on observed phenomenon and to refine it for the\ndetection system optimisation. The effect was introduced in EGS4 code system.\nThe first simulations were consecrated to different geometry of water tank in\ntotal reflection. The model was compared with experimental data realised with\ngamma source using the telescope. A simple atmospheric model is introduced in\nEGS4. The comparison between CORSIKA and EGS4 codes was realised.",
    "arxiv_id": "physics/0311044",
    "authors": [
      "I. Angelov",
      "E. Duverger",
      "E. Malamova",
      "L. Makovicka",
      "A. Mishev",
      "J. Stamenov"
    ],
    "categories": [
      "physics.comp-ph",
      "physics.ins-det"
    ],
    "title": "Modeling and Study of the Cerenkov Effect",
    "url": "https://arxiv.org/abs/physics/0311044"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "bacb4363-82ab-4abd-8ada-07c865d14764",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}