{
  "abstract": "POEMMA-Balloon with Radio (PBR) is a hybrid fluorescence and optical Cherenkov telescope that is a pathfinder instrument for a future Probe Of Extreme Multi-Messenger Astrophysics (POEMMA), together with a radio instrument, to be flown on a super pressure balloon in Spring 2028. One of its science objectives is follow up of astrophysical event alerts via signals of tau decays in the atmosphere, sourced by Earth-skimming tau neutrinos. The recent report of the KM3NeT Collaboration's muon event with $ E_μ=120^{+110}_{-60}$ PeV sparked searches for beyond the standard model (BSM) physics explanations. Using a specific, boosted dark matter scenario which together with the KM3NeT observation, sets a scale for the fluence of boosted dark matter in this energy range, we assess the capabilities of PBR to constrain or discover such a source for a boosted dark matter energy spectrum above $\\sim 10^8$ GeV. PBR has discovery potential for dark matter energies above $10^9$ GeV, and depending on BSM input parameters, to dark matter energies as low as $1.5\\times 10^8$ GeV. While the analysis is focused on one BSM example, the methodology is applicable to any BSM physics that affects tau production in the Earth.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2610.29942",
  "author_total": 121,
  "authors": [
    {
      "name": "M. H. Reno"
    },
    {
      "name": "T. Venters"
    },
    {
      "name": "M. Abrate"
    },
    {
      "name": "J. Adams"
    },
    {
      "name": "J. Alfaro"
    },
    {
      "name": "D. Allard"
    },
    {
      "name": "P. Alldredge"
    },
    {
      "name": "R. Aloisio"
    },
    {
      "name": "R. Ammendola"
    },
    {
      "name": "A. Anastasio"
    },
    {
      "name": "L. Anchordoqui"
    },
    {
      "name": "D. Badoni"
    },
    {
      "name": "J. Baláž"
    },
    {
      "name": "B. Baret"
    },
    {
      "name": "M. Battisti"
    },
    {
      "name": "R. Bellotti"
    },
    {
      "name": "M. Bertaina"
    },
    {
      "name": "M. Betts"
    },
    {
      "name": "S. Blin"
    },
    {
      "name": "M. Boezio"
    },
    {
      "name": "P. Bořil"
    },
    {
      "name": "I. Buckland"
    },
    {
      "name": "J. Burton Heibges"
    },
    {
      "name": "F. Cafagna"
    },
    {
      "name": "R. Caruso"
    },
    {
      "name": "M. Casolino"
    },
    {
      "name": "K. Černý"
    },
    {
      "name": "B. Chamanbahar"
    },
    {
      "name": "N. Cordrey"
    },
    {
      "name": "A. Creusot"
    },
    {
      "name": "A. Cummings"
    },
    {
      "name": "C. De Santis"
    },
    {
      "name": "P. Degarate"
    },
    {
      "name": "N. DeWitt Pierrat"
    },
    {
      "name": "A. Di Giovanni"
    },
    {
      "name": "A. Di Salvo"
    },
    {
      "name": "B. J. DiLella"
    },
    {
      "name": "J. Eser"
    },
    {
      "name": "S. Ferrarese"
    },
    {
      "name": "G. Filippatos"
    },
    {
      "name": "J. Ford"
    },
    {
      "name": "N. Gagalis"
    },
    {
      "name": "P. Gálvez Molina"
    },
    {
      "name": "S. Garbolino"
    },
    {
      "name": "D. Garg"
    },
    {
      "name": "R. Gargiulo"
    },
    {
      "name": "B. Gockel"
    },
    {
      "name": "A. Grelle"
    },
    {
      "name": "C. Guépin"
    },
    {
      "name": "A. Haungs"
    },
    {
      "name": "T. Heibges"
    },
    {
      "name": "J. Hinkel"
    },
    {
      "name": "A. K. Ikehara"
    },
    {
      "name": "J. Krizmanic"
    },
    {
      "name": "L. Kupari"
    },
    {
      "name": "E. H. Lenzing"
    },
    {
      "name": "F. Liberatori"
    },
    {
      "name": "S. Mackovjak"
    },
    {
      "name": "D. Mandát"
    },
    {
      "name": "M. Manfrin"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/7ajtgr1he0nhq.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2610.29942",
  "fulltext_url": null,
  "id": "7ajtgr1he0nhq",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2610.29942",
  "language": "en",
  "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": [
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      "astro-ph.HE"
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    [
      "openalex",
      "3106|Dark Matter and Cosmic Phenomena"
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  "openalex": "W7223251857",
  "pdf_url": "https://arxiv.org/pdf/2610.29942",
  "pmcid": null,
  "pmid": null,
  "published": "2026-10-27",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/7ajtgr1he0nhq.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T12:35:50Z",
      "native_id": "2610.29942",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2610.29942"
    },
    {
      "first_seen": "2026-11-04T12:20:53Z",
      "native_id": "hal-05850615",
      "source": "hal",
      "url": "https://hal.science/hal-05850615v1"
    }
  ],
  "subjects": [
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.HE",
      "subfield": "high-energy-astrophysics"
    },
    {
      "field": "physics",
      "origin": "arxiv:hep-ph",
      "subfield": "high-energy"
    }
  ],
  "title": "PBR sensitivity to boosted dark matter explanation for the KM3-230213A event",
  "title_text": "PBR sensitivity to boosted dark matter explanation for the KM3-230213A event",
  "type": "preprint",
  "updated_at": "2026-11-05T12:20:12Z",
  "url": "https://research.draconitic.com/paper/7ajtgr1he0nhq",
  "venue": "arXiv",
  "versions": []
}