{
  "id": "1011.3752",
  "version": "v1",
  "published": "2010-11-16T16:42:06.000Z",
  "updated": "2010-11-16T16:42:06.000Z",
  "title": "Core Collapse Supernovae using CHIMERA: Gravitational Radiation from Non-Rotating Progenitors",
  "authors": [
    "Konstantin Yakunin",
    "Pedro Marronetti",
    "Anthony Mezzacappa",
    "Stephen W Bruenn",
    "Ching-Tsai Lee",
    "Merek A Chertkow",
    "W Raphael Hix",
    "John M Blondin",
    "Eric J Lentz",
    "O E Bronson Messer",
    "Shin Yoshida"
  ],
  "comment": "4 pages, 1 figure, SciDAC 2010 Conference Proceedings",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "The CHIMERA code is a multi-dimensional multi-physics engine dedicated primarily to the simulation of core collapse supernova explosions. One of the most important aspects of these explosions is their capacity to produce gravitational radiation that is detectable by Earth-based laser-interferometric gravitational wave observatories such as LIGO and VIRGO. We present here preliminary gravitational signatures of two-dimensional models with non-rotating progenitors. These simulations exhibit explosions, which are followed for more than half a second after stellar core bounce.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2010-11-16T16:42:06.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "gravitational radiation",
      "non-rotating progenitors",
      "multi-physics engine dedicated primarily",
      "core collapse supernova explosions",
      "earth-based laser-interferometric gravitational wave observatories"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 877456,
      "adsabs": "2010arXiv1011.3752Y"
    }
  }
}