{
  "annotation_id": "4d476a1c-2670-4b16-8bdb-c9a433997d67",
  "date_created": "2026-03-02T18:01:17.246000Z",
  "date_modified": "2026-03-02T18:01:17.246000Z",
  "file_hash": "36b6527952e95c8a8f883307156ae80b48cd4b929e44e11f03a5c6ad8286386f",
  "private": false,
  "record": {
    "abstract": "The existence of a positive cosmological constant leads naturally to two\nfundamental scales of length, being the De Sitter horizon and the radius of the\ncell associated with a holographic degree of freedom. Associated with each of\nthose scales of length are a macroscopic gravitational mass and a microscopic\nquantum mechanical mass. Three of those four fundamental masses have been\ndiscussed in the literature, and this present work identifies the physical\nsignificance of the remaining mass, being the gravitational mass associated\nwith the holographic length. That mass, which is of the order 10^{12}kg and\ninversely proportional to the sixth root of the cosmological constant,\nrepresents the mass of the black hole whose evaporation time is equal to the\nfundamental cosmic time, which is of the order the current age of the universe.\nIt also represents the minimum mass of a black hole that is capable of\naccreting a particle whose Compton wavelength is equal to the fundamental\nholographic length, which is of the order the Compton wavelength of the\nnucleon.",
    "arxiv_id": "physics/0701289",
    "authors": [
      "Scott Funkhouser"
    ],
    "categories": [
      "physics.gen-ph"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "title": "A fundamental scale of mass for black holes from the cosmological   constant",
    "url": "https://arxiv.org/abs/physics/0701289"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "f5ae2640-3a26-489b-9838-ebd2e686bae7",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}