{
  "abstract": "We present Transient PULSE, a software package that numerically implements a previously developed source-to-detector framework for transient ultralight bosonic signals from astrophysical bursts. Predicting these signals relies on connecting the source emission spectrum to its evolution during propagation and the resulting observables at a terrestrial detector. The package discretizes a user supplied energy spectrum into momentum modes, propagates them through a specified matter density profile and constructs the time-frequency energy density distribution at Earth, accounting for dispersion and in-medium screening effects. This treatment accommodates non-Gaussian source spectra and provides inputs for detector specific analyses. A complementary analytical module estimates coupling sensitivities, arrival time delays and screening thresholds from parameterized source and detector properties.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2610.20601",
  "author_total": 5,
  "authors": [
    {
      "name": "Jason Arakawa"
    },
    {
      "name": "Charles Cheung"
    },
    {
      "name": "Muhammad Hani Zaheer"
    },
    {
      "name": "Volodymyr Takhistov"
    },
    {
      "name": "Marianna Safronova"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/8jpt1kg749qzd.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2610.20601",
  "fulltext_url": null,
  "id": "8jpt1kg749qzd",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2610.20601",
  "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",
      "astro-ph.HE"
    ],
    [
      "arxiv",
      "astro-ph.IM"
    ],
    [
      "arxiv",
      "hep-ph"
    ],
    [
      "arxiv",
      "physics.comp-ph"
    ],
    [
      "openalex",
      "3106|Dark Matter and Cosmic Phenomena"
    ]
  ],
  "openalex": "W7222187923",
  "pdf_url": "https://arxiv.org/pdf/2610.20601",
  "pmcid": null,
  "pmid": null,
  "published": "2026-10-14",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/8jpt1kg749qzd.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T12:29:31Z",
      "native_id": "2610.20601",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2610.20601"
    }
  ],
  "subjects": [
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.HE",
      "subfield": "high-energy-astrophysics"
    },
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.IM",
      "subfield": "instrumentation-methods"
    },
    {
      "field": "physics",
      "origin": "arxiv:physics.comp-ph",
      "subfield": "computational"
    },
    {
      "field": "physics",
      "origin": "arxiv:hep-ph",
      "subfield": "high-energy"
    }
  ],
  "title": "Transient PULSE: Code for the Transient Propagation of UltraLight (pseudo)Scalars to Earth",
  "title_text": "Transient PULSE: Code for the Transient Propagation of UltraLight (pseudo)Scalars to Earth",
  "type": "preprint",
  "updated_at": "2026-10-30T12:29:31Z",
  "url": "https://research.draconitic.com/paper/8jpt1kg749qzd",
  "venue": "arXiv",
  "versions": []
}