{
  "id": "1906.05935",
  "version": "v1",
  "published": "2019-06-13T21:28:56.000Z",
  "updated": "2019-06-13T21:28:56.000Z",
  "title": "Study of PeV neutrinos around dwarf galaxies near giant lobes of Centaurus A",
  "authors": [
    "E. Aguilar-Ruiz",
    "N. Fraija",
    "A. Galván-Gámez",
    "J. A. De Diego",
    "A. Marinelli"
  ],
  "comment": "To appear in the Proceedings of the XV International Conference on Topics in Astroparticle and Underground Physics (TAUP2017) at Journal of Physics: Conference Series (JPCS)",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "The origin of recently discovered PeV neutrinos is an unsolved problem. In this work we consider a hadronic scenario to produce PeV neutrinos from a region around giant lobes of Centaurus A. Although ultrahigh-energy cosmic rays (UHECRs) are accelerated and confined by giant lobes, they can escape to be later injected in the inter-group medium where galaxies near the giant lobes provides the condition to confine them. UHECRs interact with low-energy photons and protons producing high-energy photons and neutrinos. We found that the IC35 event cannot be generated neither inside the giant lobes nor galaxies close to the lobes of Centaurus A.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2019-06-13T21:28:56.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "giant lobes",
      "dwarf galaxies",
      "protons producing high-energy photons",
      "produce pev neutrinos",
      "ultrahigh-energy cosmic rays"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}