{
  "annotation_id": "7167461c-7f14-4eb4-b3ca-398512676f73",
  "date_created": "2026-03-02T18:02:10.164000Z",
  "date_modified": "2026-03-02T18:02:10.164000Z",
  "file_hash": "845b63757420a10255b9fe07dcc0b35cf2f2da9d99a4dbe88142e9c9c6ba89a7",
  "private": false,
  "record": {
    "abstract": "We give a relativistically covariant, wave-functional formulation of Bohm\u0027s\nquantum field theory for the scalar field based on a general foliation of\nspace-time by space-like hypersurfaces. The wave functional, which guides the\nevolution of the field, is space-time-foliation independent but the field\nitself is not. Hence, in order to have a theory in which the field may be\nconsidered a beable, some extra rule must be given to determine the foliation.\nWe suggest one such rule based on the eigen vectors of the energy-momentum\ntensor of the field itself.",
    "arxiv_id": "quant-ph/0407089",
    "authors": [
      "George Horton",
      "Chris Dewdney"
    ],
    "categories": [
      "quant-ph"
    ],
    "doi": "10.1088/0305-4470/37/49/011",
    "journal_ref": "J.Phys. A37 (2004) 11935-11944",
    "title": "A relativistically covariant version of Bohm\u0027s quantum field theory for   the scalar field",
    "url": "https://arxiv.org/abs/quant-ph/0407089"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "69dbf7e6-be1c-45d3-845a-fec1bba48227",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}