{
  "abstract": "In this manuscript, a dynamical inverse seesaw neutrino ISS(3+1+1+1) mixing model based on the gauge symmetry $U(1)_{B-L}$ extended by the flavor symmetry $A_{4}\\times Z_{2}$ has been constructed. ISS(3+1+1+1) represents three generations of right-handed neutrinos and an extra three generation of singlets sterile neutrinos, wherein the right-handed neutrinos are triplets under $A_4$ symmetry. Furthermore, the five scalar flavon fields are considered in the model, which reproduce neutrino oscillation data within the NuFIT 6.0 experimental range with statistical $\\text{|pull|}=0.01 σ$. The neutrino mass hierarchy is obtained by minimizing the dynamical $A_4\\times Z_2$ scalar flavon $ϕ_v$ potential. The effective neutrino mass parameter $m_{ββ}$ for the neutrinoless double beta decay $0vββ$ has been charecterised in the manuscript. The effective neutrino mass parameter spans a finite region in the parameter space rather then being confined to a single point and it is constrained by the KamLAND-Zen excluded band. The model successfully explains active-sterile neutrino mixing and non-unitarity of the PMNS matrix is consistent with the cosmological upper bound. The minimum value of the sum of the active neutrinos' mass turns out to be $m_{i}\\approx 62\\ \\ (99.4)\\ \\text{meV}$ for Normal ordering (Inverted ordering), which lies within the range of both Planck 2018 loose cosmological limit $\\sum m_{i}<120\\ \\text{meV}$ and tighter limit $\\sum m_{i}<72\\ \\text{meV}$ of DESI-2024. Our model immensely favours normal ordering, in agreement with the tighter constraints reported by DESI-2024.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2610.30981",
  "author_total": 4,
  "authors": [
    {
      "name": "Manish Singh Bisht"
    },
    {
      "name": "Shuchi Bisht"
    },
    {
      "name": "Mayank Joshi"
    },
    {
      "name": "Navjot Hothi"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/fj2ngwz0ybp56.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2610.30981",
  "fulltext_url": null,
  "id": "fj2ngwz0ybp56",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2610.30981",
  "language": null,
  "licence": "CC-BY-SA-4.0",
  "licence_label": "CC BY-SA 4.0",
  "licence_source": "article",
  "licence_url": "http://creativecommons.org/licenses/by-sa/4.0/",
  "metadata_licence": "CC0-1.0",
  "native_subjects": [
    [
      "arxiv",
      "gr-qc"
    ],
    [
      "arxiv",
      "hep-ph"
    ],
    [
      "openalex",
      "3106|Neutrino Physics Research"
    ]
  ],
  "openalex": "W7223380563",
  "pdf_url": "https://arxiv.org/pdf/2610.30981",
  "pmcid": null,
  "pmid": null,
  "published": "2026-10-22",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/fj2ngwz0ybp56.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T12:34:34Z",
      "native_id": "2610.30981",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2610.30981"
    }
  ],
  "subjects": [
    {
      "field": "physics",
      "origin": "arxiv:gr-qc",
      "subfield": "gravitation"
    },
    {
      "field": "physics",
      "origin": "arxiv:hep-ph",
      "subfield": "high-energy"
    }
  ],
  "title": "Construction and phenomenological analysis of dynamical Inverse seesaw neutrino mixing model",
  "title_text": "Construction and phenomenological analysis of dynamical Inverse seesaw neutrino mixing model",
  "type": "preprint",
  "updated_at": "2026-10-30T12:34:34Z",
  "url": "https://research.draconitic.com/paper/fj2ngwz0ybp56",
  "venue": "arXiv",
  "versions": []
}