{
  "annotation_id": "938f830c-30ec-4aa4-8708-684cd9a511d5",
  "date_created": "2026-03-02T18:00:36.236000Z",
  "date_modified": "2026-03-02T18:00:36.236000Z",
  "file_hash": "7461aaf54788a1fbcd2080abb0b91abe6cbfd7f7e447ff9c793ca242d2114982",
  "private": false,
  "record": {
    "abstract": "The relativistic corrections to the Maxwellian velocity distribution are\nneeded for standard solar models. Relativistic equilibrium velocity\ndistribution, if adopted in standard solar models, will lower solar neutrino\nfluxes and change solar neutrino energy spectra but keep solar sound speeds. It\nis possibly a solution to the solar neutrino problem.",
    "arxiv_id": "physics/0110002",
    "authors": [
      "Jian-Miin Liu"
    ],
    "categories": [
      "physics.gen-ph"
    ],
    "title": "A possible solution to the solar neutrino problem: Relativistic   corrections to the Maxwellian velocity distribution",
    "url": "https://arxiv.org/abs/physics/0110002"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "f24f3d4f-7cf2-459f-b050-41ba9193bc9a",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}