{
  "annotation_id": "3d68f1e4-6edc-4a7a-bb7f-157479a4ed13",
  "date_created": "2026-03-02T18:02:05.751000Z",
  "date_modified": "2026-03-02T18:02:05.751000Z",
  "file_hash": "d89212955e73a5e2229c89c578007df517bab5af558705673d7cfb009ea06758",
  "private": false,
  "record": {
    "abstract": "A detector undergoing uniform acceleration $a$ in a vacuum field responds\njust as though it were immersed in thermal radiation of temperature $T=\\hbar\na/2\\pi k c$. A simple, intuitive derivation of this result is given for the\ncase of a scalar field in one spatial dimension. The approach is then extended\nto treat the case where the field seen by the accelerated observer is a\nspin-1/2 Dirac field.",
    "arxiv_id": "quant-ph/0401170",
    "authors": [
      "Paul M. Alsing",
      "Peter W. Milonni"
    ],
    "categories": [
      "quant-ph",
      "gr-qc"
    ],
    "doi": "10.1119/1.1761064",
    "journal_ref": "Am.J.Phys. 72 (2004) 1524-1529",
    "title": "Simplified derivation of the Hawking-Unruh temperature for an   accelerated observer in vacuum",
    "url": "https://arxiv.org/abs/quant-ph/0401170"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "749d1db1-1b09-4bf6-9470-a9e43a153811",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}