{
  "annotation_id": "710cd588-5f05-4ff0-89a0-6cc772d749ce",
  "date_created": "2026-03-02T18:01:42.076000Z",
  "date_modified": "2026-03-02T18:01:42.076000Z",
  "file_hash": "b0fff0745e0f68e67dc32f858a8f03cb990101213df0ebb43ede01b4dee2b41e",
  "private": false,
  "record": {
    "abstract": "Quantum spin-flip transitions are of great importance in the synchrotron\nradiation theory. For better understanding of the nature of this phenomenon, it\nis necessary to except the effects connected with the electric charge radiation\nfrom observation. This fact explains the suggested choice of the spin-flip\nradiation model in the form of radiation of the electric neutral Dirac-Pauli\nparticle moving in the homogeneous magnetic field. It is known that in this\ncase, the total radiation in the quantum theory is conditioned by spin-flip\ntransitions. The idea is that spin-flip radiation is represented as a\nnonstationary process connected with spin precession. We shall shown how to\nconstruct a solution of the classical equation of the spin precession in the\nBMT theory having the exact solution of the Dirac-Pauli equation.Thus, one will\nfind the connection of the quantum spin-flip transitions with classical spin\nprecession.",
    "arxiv_id": "quant-ph/0102063",
    "authors": [
      "V. A. Bordovitsyn",
      "V. S. Gushchina",
      "A. N. Myagkii"
    ],
    "categories": [
      "quant-ph"
    ],
    "doi": "10.1016/S0168-9002(97)01048-6",
    "journal_ref": "Nucl. Instr. and Meth. A405 (1998) 256-257",
    "title": "Discussion on spin-flip synchrotron radiation",
    "url": "https://arxiv.org/abs/quant-ph/0102063"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "af39f2a1-d7b4-48fb-afbd-1775c605a520",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}