{
  "annotation_id": "25402ff3-de24-4c31-afc6-b9ad7a5a9ca5",
  "date_created": "2026-03-02T18:00:01.132000Z",
  "date_modified": "2026-03-02T18:00:01.132000Z",
  "file_hash": "55826ab2cd3a4c296d66921244a2e1a12c1195bd67592a2d4474561884c9e4e3",
  "private": false,
  "record": {
    "abstract": "We study neutral current neutrino-nucleus reaction cross-sections for Mn, Fe,\nCo and Ni isotopes. An earlier study for a few selected nuclei has shown that\nin the supernova environment the cross sections are increased for low energy\nneutrinos due to finite-temperature effects. Our work supports this finding for\na much larger set of nuclei. Furthermore we extend previous work to higher\nneutrino energies considering allowed and forbidden multipole contributions to\nthe cross sections. The allowed contributions are derived from large-scale\nshell model calculations of the Gamow-Teller strength, while the other\nmultipole contributions are calculated within the Random Phase Approximation.\nWe present the cross sections as functions of initial and final neutrino\nenergies and for a range of supernova-relevant temperatures. These cross\nsections will allow improved estimates of inelastic neutrino reactions on\nnuclei in supernova simulations.",
    "arxiv_id": "nucl-th/0404078",
    "authors": [
      "A. Juodagalvis",
      "K. Langanke",
      "G. Martinez-Pinedo",
      "W. R. Hix",
      "D. J. Dean",
      "J. M. Sampaio"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/j.nuclphysa.2004.09.005",
    "journal_ref": "Nucl.Phys. A747 (2005) 87-108",
    "title": "Neutral-current neutrino-nucleus cross-sections for A~50-65 nuclei",
    "url": "https://arxiv.org/abs/nucl-th/0404078"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "001f5109-aadf-4c93-9119-39ce1d87dc2e",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}