{
  "annotation_id": "b6adad07-f1c5-41f2-88ee-3d1361cf66b3",
  "date_created": "2026-03-02T18:00:25.479000Z",
  "date_modified": "2026-03-02T18:00:25.479000Z",
  "file_hash": "ed2a4e599fd2d150297e91176cd42f43574e8896872fa244691e42ea1fd2225a",
  "private": false,
  "record": {
    "abstract": "These lectures cover three topics in neutrino astrophysics. The solar\nneutrino problem is reviewed, with particular emphasis on the microphysics of\nthe standard solar model, detector responses, the quantum mechanics of the MSW\nmechanism, and the possibility of spin-flavor oscillations. In the second\nlecture the electromagnetic properties of Dirac and Majorana neutrinos are\ndiscussed. Two classic problems in red giant evolution - the triple alpha\nreaction and the delay of the He flash by anomalous cooling - are used to\nillustrate how stellar cooling arguments constrain neutrino properties. Axion\nand Dirac neutrino mass effects on supernova cooling are also discussed. The\nthird lecture describes the supernova explosion mechanism and the associated\nnucleosynthesis. The neutrino process and r-process are discussed, including\nthe \"neutrino fingerprint\" on the latter that supports earlier suggestions that\nthe r-process site is near the mass cut of a type II supernova. The effects of\ntau neutrino oscillations on the r-process are described briefly. The material\nis presented at a level suitable for graduate students at the beginning of\ntheir research careers.",
    "arxiv_id": "nucl-th/9901076",
    "authors": [
      "W. C. Haxton"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "hep-ph"
    ],
    "doi": "10.1142/9789812813497_0007",
    "title": "Topics in Neutrino Astrophysics",
    "url": "https://arxiv.org/abs/nucl-th/9901076"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "cbc71294-4bab-4d1f-9f12-c99839a7cc4b",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}