{
  "annotation_id": "3c8f1cbb-cd17-49ac-b2e5-28bfeeb206d4",
  "date_created": "2026-03-02T18:01:42.702000Z",
  "date_modified": "2026-03-02T18:01:42.702000Z",
  "file_hash": "a5e383ae1431a7e9a7664a9570e1c16c4953d4068588d46a516b21f45813b274",
  "private": false,
  "record": {
    "abstract": "Alternative to the sonic black hole analogues we discuss a different scenario\nfor modeling the Schwarzschild geometry in a laboratory - the dielectric black\nhole. The dielectric analogue of the horizon occurs if the velocity of the\nmedium with a finite permittivity exceeds the speed of light in that medium.\nThe relevance for experimental tests of the Hawking effect and possible\nimplications are addressed. PACS: 04.70.Dy, 04.62.+v, 04.80.-y, 42.50.Gy.",
    "arxiv_id": "quant-ph/0104121",
    "authors": [
      "Ralf Sch\u00fctzhold",
      "G\u00fcnter Plunien",
      "Gerhard Soff"
    ],
    "categories": [
      "quant-ph"
    ],
    "doi": "10.1103/PhysRevLett.88.061101",
    "journal_ref": "Phys.Rev.Lett. 88 (2002) 061101",
    "title": "Dielectric black hole analogues",
    "url": "https://arxiv.org/abs/quant-ph/0104121"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "e73270d1-741e-4ad3-a17f-6c4eecd13bf9",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}