{
  "abstract": "Many important charge-exchange weak processes, such as beta decays, double beta decays, and neutrino-nucleus and neutrino-nucleon reactions, are closely related to the spin- and isospin-dependent nuclear force, yet few of them can be precisely measured, or even observed, in terrestrial experiments. The Gamow-Teller resonance (GTR) in finite nuclei is one of the few experimental probes of this spin-isospin force. In a companion letter, we obtained the probability distribution of the Landau-Migdal parameter $G'_0$, which characterizes the main part of the spin-isospin force, from GTR measurements using Bayesian inference. In this follow-up work, we quantitatively study the correlations emerging from this Bayesian analysis. From the posterior, we identify two standard Skyrme parameterizations (nuSky*) that reproduce, in a unified manner, ground-state observables of finite nuclei, the salient features of the GTR, and the bulk properties of neutron-star matter. Since collective excitations in finite nuclei and in neutron-star matter are related, we use the Skyrme interactions sampled from the posterior to constrain the axial-current, charged-current neutrino-nucleon reaction rates in hot and dense compact-star matter, as the first astrophysical application of this study. The GTR-informed calculations substantially reduce the spread of the neutrino opacity; nevertheless, significant uncertainties remain due to the poorly constrained symmetry energy at sub-saturation densities. Constraining this quantity on top of a well-constrained spin-isospin interaction would pave the way towards a systematic determination of neutrino interactions in dense matter.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2611.05153",
  "author_total": 4,
  "authors": [
    {
      "name": "Zidu Lin"
    },
    {
      "name": "Gianluca Colò"
    },
    {
      "name": "Andrew W. Steiner"
    },
    {
      "name": "Amber Stinson"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/c3rw95k7jax7t.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2611.05153",
  "fulltext_url": null,
  "id": "c3rw95k7jax7t",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2611.05153",
  "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",
      "nucl-th"
    ]
  ],
  "openalex": null,
  "pdf_url": "https://arxiv.org/pdf/2611.05153",
  "pmcid": null,
  "pmid": null,
  "published": "2026-11-03",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/c3rw95k7jax7t.ris",
  "sources": [
    {
      "first_seen": "2026-11-04T15:21:25Z",
      "native_id": "2611.05153",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2611.05153"
    }
  ],
  "subjects": [
    {
      "field": "physics",
      "origin": "arxiv:nucl-th",
      "subfield": "nuclear"
    }
  ],
  "title": "Information content of the Gamow Teller Resonance: Bayesian inference with self-consistent Skyrme models",
  "title_text": "Information content of the Gamow Teller Resonance: Bayesian inference with self-consistent Skyrme models",
  "type": "preprint",
  "updated_at": "2026-11-06T18:21:01Z",
  "url": "https://research.draconitic.com/paper/c3rw95k7jax7t",
  "venue": "arXiv",
  "versions": []
}