{
  "abstract": "We present an improved parametric model for neutrino emission from core-collapse supernovae that directly connects neutrino luminosity and average energy to stellar properties during emission. Our model incorporates two critical physical processes: convection within the proto-neutron star and the evolution of the neutrinosphere radius during the early emission phase. Using simulated datasets of supernova neutrino events in the Super-Kamiokande detector, we assess the sensitivity to astrophysical properties in the event of a future detection. We show that the neutrino mass ordering plays a crucial role in determining which parameters can be constrained by the observed neutrino data.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2610.12101",
  "author_total": 5,
  "authors": [
    {
      "name": "Matteo Ballelli"
    },
    {
      "name": "Federica Pompa"
    },
    {
      "name": "Christoph Ternes"
    },
    {
      "name": "Marco Drago"
    },
    {
      "name": "Giulia Pagliaroli"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/5btwcwg4p3b4c.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2610.12101",
  "fulltext_url": null,
  "id": "5btwcwg4p3b4c",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2610.12101",
  "language": null,
  "licence": "LicenseRef-arXiv-nonexclusive-1.0",
  "licence_label": "arXiv licence",
  "licence_source": "article",
  "licence_url": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
  "metadata_licence": "CC0-1.0",
  "native_subjects": [
    [
      "arxiv",
      "astro-ph.HE"
    ],
    [
      "arxiv",
      "astro-ph.SR"
    ],
    [
      "arxiv",
      "hep-ph"
    ],
    [
      "openalex",
      "3106|Neutrino Physics Research"
    ]
  ],
  "openalex": "W7221195153",
  "pdf_url": "https://arxiv.org/pdf/2610.12101",
  "pmcid": null,
  "pmid": null,
  "published": "2026-10-08",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/5btwcwg4p3b4c.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T12:27:54Z",
      "native_id": "2610.12101",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2610.12101"
    }
  ],
  "subjects": [
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.HE",
      "subfield": "high-energy-astrophysics"
    },
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.SR",
      "subfield": "stellar"
    },
    {
      "field": "physics",
      "origin": "arxiv:hep-ph",
      "subfield": "high-energy"
    }
  ],
  "title": "An updated model of neutrino emission from proto-neutron stars",
  "title_text": "An updated model of neutrino emission from proto-neutron stars",
  "type": "preprint",
  "updated_at": "2026-10-30T12:27:54Z",
  "url": "https://research.draconitic.com/paper/5btwcwg4p3b4c",
  "venue": "arXiv",
  "versions": []
}