{
  "annotation_id": "8f993428-46c6-4fa2-9e19-f8a600028d68",
  "date_created": "2026-03-02T17:59:57.653000Z",
  "date_modified": "2026-03-02T17:59:57.653000Z",
  "file_hash": "f010c8797e5868fa67cb58dbdda7df1f5e31a7dc1805b5401faf64945a7ada03",
  "private": false,
  "record": {
    "abstract": "I describe how the signals corresponding to the supernova $\\nu_e$ and\n$\\bar{\\nu}_e$ (charged current reactions) as well as all active neutrinos\n(neutral current reactions) can be separately observed in various existing\ndetectors. These observations would make it possible to determine the flux and\naverage energy (or temperature) for each of these three neutrino signal\ncomponents. I argue that all these quantities are needed in order to understand\nthe interplay between the so far poorly known supernova neutrino emission\nprocess and the neutrino oscillations.",
    "arxiv_id": "nucl-th/0305003",
    "authors": [
      "Petr Vogel"
    ],
    "categories": [
      "nucl-th"
    ],
    "title": "Supernova Neutrinos",
    "url": "https://arxiv.org/abs/nucl-th/0305003"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "a7014315-dd06-446e-9bc5-9cbb59dc96b4",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}