{
  "annotation_id": "d3e730ba-a3e8-4423-abc0-1c38bf0a0de0",
  "date_created": "2026-03-02T18:00:56.382000Z",
  "date_modified": "2026-03-02T18:00:56.382000Z",
  "file_hash": "bd6b10d691a4b860a383af468ac837726f27fa1ccc130c018c5055cfe62d407b",
  "private": false,
  "record": {
    "abstract": "Relying on the obtained results in Rev.[1](physics/0505035), we derive the\nformula relating the red-shift of light signals coming from distant galaxies to\nthe distance of these galaxies from us and the time of detecting of these light\nsignals. The red-shift coefficient, instead of the Hubble parameter, is\nintroduced. It varies with time and positive at all times. Its nowadays value\nequals the Hubble parameter. It increases forever as time is running from the\npast to the future. The derived formula enables us to estimate the nowadays\nincreasing rate of the red-shift coefficient, which is nothing but the nowadays\nvalue of the \"acceleration of the expansion of the Universe\".",
    "arxiv_id": "physics/0505036",
    "authors": [
      "Jian-Miin Liu"
    ],
    "categories": [
      "physics.gen-ph"
    ],
    "title": "Formula for red-shift of light signals coming from distant galaxies",
    "url": "https://arxiv.org/abs/physics/0505036"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "8a7c4fdf-436b-4026-b7a7-5ca1589e4c09",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}