{
  "annotation_id": "e0e3369a-f716-4a64-bff5-c4d2f52b39e9",
  "date_created": "2026-03-02T18:02:10.378000Z",
  "date_modified": "2026-03-02T18:02:10.378000Z",
  "file_hash": "f57b5ff45a6ebd946e36f858cd1fd080e626dad036f5800aeb6f3d04cc390db3",
  "private": false,
  "record": {
    "abstract": "It is demonstrated that the propagation of electro-magnetic waves in an\nappropriately designed wave-guide is (for large wave-lengths) analogous to that\nwithin a curved space-time -- such as around a black hole. As electro-magnetic\nradiation (e.g., micro-weaves) can be controlled, amplified, and detected (with\npresent-day technology) much easier than sound, for example, we propose a\nset-up for the experimental verification of the Hawking effect. Apart from\nexperimentally testing this striking prediction, this would facilitate the\ninvestigation of the trans-Planckian problem. PACS: 04.70.Dy, 04.80.-y,\n42.50.-p, 84.40.Az.",
    "arxiv_id": "quant-ph/0408145",
    "authors": [
      "Ralf Sch\u00fctzhold",
      "William G. Unruh"
    ],
    "categories": [
      "quant-ph",
      "gr-qc"
    ],
    "doi": "10.1103/PhysRevLett.95.031301",
    "journal_ref": "Phys.Rev.Lett. 95 (2005) 031301",
    "title": "Hawking radiation in an electro-magnetic wave-guide?",
    "url": "https://arxiv.org/abs/quant-ph/0408145"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "b62960dc-935c-43d5-8788-929fa574ffae",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}