{
  "id": "2401.06304",
  "version": "v1",
  "published": "2024-01-12T00:20:37.000Z",
  "updated": "2024-01-12T00:20:37.000Z",
  "title": "A Unified Model for Multi-epoch Neutrino Events and Broadband Spectral Energy Distribution of $\\rm TXS~0506+056$",
  "authors": [
    "Zhen-Jie Wang",
    "Ruo-Yu Liu",
    "Ze-Rui Wang",
    "Junfeng Wang"
  ],
  "comment": "19pages,12figures,accepted for publication in ApJ. arXiv admin note: text overlap with arXiv:2211.07070",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "The blazar $TXS~0506+056$ has been proposed as a high-energy neutrino emitter. However, it has been shown that the standard one-zone model cannot produce sufficiently high neutrino flux due to constraints from the X-ray data, implying more complex properties of the radiation zones in the blazar than that described by the standard one-zone model. In this work we investigate multi-epoch high-energy muon neutrino events associated with the blazar $TXS~0506+056$ occured in 2014-2015, 2017-2018, 2021-2022 and 2022-2023, respectively. We applied the so-called ``stochastic dissipation model'' to account for the neutrino-blazar associations detected in the four epochs simultaenously. This model describes a scenario in which the emission of the blazar arise from the superimposition of two components: a persistent component related to the quasi-stable state of the blazar and a transient component responsible for the sudden enhancement of the blazar's flux, either in electromagnetic radiation or in neutrino emission. The latter component could form at a random distance along the jet by a strong energy dissipation event. Under such assumption, the multi-epoch broadband spectral energy distribution (SED) can be well explained and the expected number of high-energy neutrino events is statistically realistic. The expected number of neutrino events in half-year is around 8.2, 0.07, 0.73 and 0.41, corresponding to the epoch in 2014-2015, 2017-2018, 2021-2022 and 2022-2023, respectively. Hence, our model self-consistently explains the episodic neutrino emission from $TXS~0506+056$.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2024-01-12T00:20:37.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "broadband spectral energy distribution",
      "multi-epoch neutrino events",
      "high-energy muon neutrino events",
      "unified model",
      "sufficiently high neutrino flux"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 19,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}