{
  "abstract": "We extend the horizon wave-function (HWF) formalism to a spherically symmetric, charged, spinless quantum source in $\\mathcal{D} + 1$ dimensional spacetime geometry and construct the HWFs associated with inner- as well as outer-horizons of the Tangherlini--Reissner--Nordström (TRN) black hole. The corresponding black hole formation probabilities, $P_{\\rm BH}^{\\pm}$, are also calculated and their sensitivities due to various source parameters including charge, mass, and $\\mathcal{D}$ are analysed as well. Our analysis reveals that the ratio of inner- to outer-horizon probabilities, $P_{\\rm BH}^{-}/P_{\\rm BH}^{+}$, changes drastically from being unity as the source departs away from being in the extremal limit defined by $α$ ($\\to 1$ for extremal case). Furthermore, black hole formation probabilities are found to be highly suppressed for higher values of $\\mathcal{D}$, particularly for the source mass, $m \\lesssim Λ_{\\mathcal{D}}$, e.g., for $α= 0.5$, the ratio, $P_{\\rm BH}^{+}(\\mathcal{D} = 5)/P_{\\rm BH}^{+}(\\mathcal{D}=10)$ turn out to be approximately associated with $\\mathcal{D}$ spatial-dimensions.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2610.39757",
  "author_total": 3,
  "authors": [
    {
      "name": "Ashfaque Ahmad"
    },
    {
      "name": "Sudhir Kumar Gupta"
    },
    {
      "name": "Abbas Ali"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/0s4egcfvgnxhy.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2610.39757",
  "fulltext_url": null,
  "id": "0s4egcfvgnxhy",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2610.39757",
  "language": null,
  "licence": "CC-BY-4.0",
  "licence_label": "CC BY 4.0",
  "licence_source": "article",
  "licence_url": "http://creativecommons.org/licenses/by/4.0/",
  "metadata_licence": "CC0-1.0",
  "native_subjects": [
    [
      "arxiv",
      "gr-qc"
    ],
    [
      "arxiv",
      "hep-ph"
    ],
    [
      "arxiv",
      "hep-th"
    ]
  ],
  "openalex": null,
  "pdf_url": "https://arxiv.org/pdf/2610.39757",
  "pmcid": null,
  "pmid": null,
  "published": "2026-10-29",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/0s4egcfvgnxhy.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T12:36:23Z",
      "native_id": "2610.39757",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2610.39757"
    }
  ],
  "subjects": [
    {
      "field": "physics",
      "origin": "arxiv:gr-qc",
      "subfield": "gravitation"
    },
    {
      "field": "physics",
      "origin": "arxiv:hep-ph",
      "subfield": "high-energy"
    }
  ],
  "title": "HWF Analysis of TRN Black Holes",
  "title_text": "HWF Analysis of TRN Black Holes",
  "type": "preprint",
  "updated_at": "2026-11-04T15:20:51Z",
  "url": "https://research.draconitic.com/paper/0s4egcfvgnxhy",
  "venue": "arXiv",
  "versions": []
}