{
  "annotation_id": "8a6f8744-028e-465a-ab5a-14f2008041a8",
  "date_created": "2026-03-02T18:00:35.806000Z",
  "date_modified": "2026-03-02T18:00:35.806000Z",
  "file_hash": "a9075a58b24b785a907909407b1daf9262e7f15b8678e6261d9f1eb12f63843e",
  "private": false,
  "record": {
    "abstract": "A new conceptual approach for examining the origin of cosmic rays is\ndeveloped by considering the characteristics of particle trajectory\ndistributions in four-dimensional Euclidean space-time. Transformation of an\nisotropic distribution into a velocity distribution in ordinary\nthree-dimensional space results in a spatially isotropic flux of highly\nrelativistic particles. This particle flux exhibits a power-law energy spectrum\nthat decreases with increasing energy approximately inversely as the square of\nthe energy and peaks at much lower energies. This model also provides\nadditional results resembling the observed characteristics of cosmic radiation.",
    "arxiv_id": "physics/0108049",
    "authors": [
      "C. L. Herzenberg"
    ],
    "categories": [
      "physics.gen-ph"
    ],
    "doi": "10.4006/1.3025478",
    "journal_ref": "Phys.Essays 14 (2001) 171-176",
    "title": "Examining the Origin of Cosmic Rays: A New Conceptual Approach",
    "url": "https://arxiv.org/abs/physics/0108049"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "f073bd74-f4b6-4ce7-b2a6-f86d1e51dee1",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}