{
  "id": "2202.11265",
  "version": "v1",
  "published": "2022-02-23T01:46:24.000Z",
  "updated": "2022-02-23T01:46:24.000Z",
  "title": "Central black hole mass in the distant tidal disruption event candidate of {\\it Swift} J2058.4+0516",
  "authors": [
    "Zhang XueGuang"
  ],
  "comment": "10 pages, 7 figures, 1 table, Accepted to be published in ApJ",
  "categories": [
    "astro-ph.HE",
    "astro-ph.GA"
  ],
  "abstract": "In the manuscript, central black hole (BH) mass is estimated in the distant TDE (tidal disruption event) of {\\it Swift} J2058.4+0516 as the second candidate of relativistic jet birth related to TDE. {\\it Swift} J2058.4+0516 have quite different BH masses estimated through different indirect methods in the literature. Therefore, it is necessary and interesting to determine the central BH mass in {\\it Swift} J2058.4+0516 by one another independent method. Here, based on the theoretical TDE model applied to describe the long-term time-dependent X-ray variabilities of {\\it Swift} J2058.4+0516, the central BH mass can be well determined to be around $1.05_{-0.29}^{+0.39}\\times10^5{\\rm M_\\odot}$, after kind considerations of suggested intrinsic beaming effects from such relativistic jet tightly related to TDE. Moreover, the {\\it Swift} J2058.4+0516 is an unique object in the space of BH masses versus energy transfer efficiencies of the reported TDE candidates, providing interesting clues to detect and/or anticipate candidates of relativistic TDE to make the birth of relativistic jets.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2022-02-23T01:46:24.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "distant tidal disruption event candidate",
      "central black hole mass",
      "bh mass",
      "relativistic jet"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 10,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}