{
  "annotation_id": "ece91611-ab34-47ce-b235-365fe0aec11e",
  "date_created": "2026-03-02T18:01:00.582000Z",
  "date_modified": "2026-03-02T18:01:00.582000Z",
  "file_hash": "4d20809d78166f6243be2e74fc4c297c10598ae351806a67a248c2b1e2e4b88a",
  "private": false,
  "record": {
    "abstract": "The simplest possible equation for Hawking radiation, and other black hole\nradiated power is derived in terms of black hole density. Black hole density\nalso leads to the simplest possible model of a gas of elementary constituents\nconfined inside a gravitational bottle of Schwarzchild radius at tremendous\npressure, which yields identically the same functional dependence as the\ntraditional black hole entropy. Variations of Sbh can be obtained which depend\non the occupancy of phase space cells. A relation is derived between the\nconstituent momenta and the black hole radius which is similar to the Compton\nwavelength relation.",
    "arxiv_id": "physics/0506029",
    "authors": [
      "Mario Rabinowitz"
    ],
    "categories": [
      "physics.gen-ph"
    ],
    "doi": "10.1007/s10773-006-9075-6",
    "journal_ref": "Int.J.Theor.Phys. 45 (2006) 851-858",
    "title": "Black Hole Radiation and Volume Statistical Entropy",
    "url": "https://arxiv.org/abs/physics/0506029"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "e67f8664-45cf-483b-a00f-934bcbc2047a",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}