{
  "id": "2110.15620",
  "version": "v1",
  "published": "2021-10-29T08:36:44.000Z",
  "updated": "2021-10-29T08:36:44.000Z",
  "title": "Joint Analysis Method on Gravitational Waves and Low-Energy Neutrinos to Detect Core-Collapse Supernovae",
  "authors": [
    "O Halim",
    "C Casentini",
    "M Drago",
    "V Fafone",
    "K Scholberg",
    "C F Vigorito",
    "G Pagliaroli"
  ],
  "comment": "17 pages, Proceedings of the 16th Marcel Grossmann meeting held on July 5-10, 2021",
  "categories": [
    "astro-ph.HE",
    "astro-ph.IM",
    "gr-qc",
    "hep-ex"
  ],
  "abstract": "Core-collapse supernovae produce copious low-energy neutrinos and are also predicted to radiate gravitational waves. These two messengers can give us information regarding the explosion mechanism. The gravitational wave detection from these events are still elusive even with the already advanced detectors. Here we give a concise and timely introduction to a new method that combines triggers from GW and neutrino observatories; more details shall be given in a forthcoming paper [1]. Keywords: multimessenger, supernova, core-collapse, low-energy neutrino, gravitational wave.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2021-10-29T08:36:44.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "gravitational wave",
      "detect core-collapse supernovae",
      "joint analysis method",
      "core-collapse supernovae produce copious low-energy",
      "supernovae produce copious low-energy neutrinos"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 17,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}