{
  "annotation_id": "06b1cf8b-b8ca-4744-9fe6-3896e5174462",
  "date_created": "2026-03-02T18:02:37.288000Z",
  "date_modified": "2026-03-02T18:02:37.288000Z",
  "file_hash": "dfdad587c00179b244c6e83c05b2d3afb1156e8f5ccc636ff4805f993db76772",
  "private": false,
  "record": {
    "abstract": "We interpret the probability rule of the CSL collapse theory to mean that the\nscalar field which causes collapse is the grvitational curvature scalar with\ntwo sources, the expectation value of the mass density and a white noise\nfluctuating source. We examine two models of the fluctuating source, monopole\nfluctuations and dipole fluctuations, and show that these correspond to two\nwell known collapse models. We relate the two GRW parameters of CSL to\nfundamental constants, and explain the energy increase as arising from the loss\nof vacuum gravitational energy. It is shown how a problem with semi-classical\ngrvity may be cured when it is combined with a CSL collapse model.",
    "arxiv_id": "quant-ph/9503019",
    "authors": [
      "Philip Pearle",
      "Euan Squires"
    ],
    "categories": [
      "quant-ph"
    ],
    "doi": "10.1007/BF02069474",
    "title": "Gravity, energy conservation and parameter values in collapse models",
    "url": "https://arxiv.org/abs/quant-ph/9503019"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "8feaa65e-fa4c-4597-90bf-1e4d51409483",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}