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How loud are neutron star mergers?

Bernuzzi, Sebastiano; Radice, David; Ott, Christian D.; Roberts, Luke F.; Mösta, Philipp; Galeazzi, Filippo


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  "@id": "https://doi.org/10.5281/zenodo.57844", 
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  "creator": [
    {
      "@type": "Person", 
      "affiliation": "Parma U & INFN", 
      "name": "Bernuzzi, Sebastiano"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Caltech", 
      "name": "Radice, David"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Caltech", 
      "name": "Ott, Christian D."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Caltech", 
      "name": "Roberts, Luke F."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Berkeley", 
      "name": "M\u00f6sta, Philipp"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Frankfurth Goethe  U", 
      "name": "Galeazzi, Filippo"
    }
  ], 
  "datePublished": "2016-07-12", 
  "description": "<p>We release neutron star merger waveforms computed using fully general relativistic simulations of equal and unequal-mass binaries drawn from the galactic population. The simulations employ finite-temperature microphysical equations of state (LS220, DD2, and SFHo) and neutrino cooling. Please, see</p>\n\n<p>http://arxiv.org/abs/1512.06397</p>\n\n<p>for details.</p>\n\n<p>&nbsp;</p>\n\n<p>Each tarball refers to a simulation and contains</p>\n\n<ul>\n\t<li>Curvature multipolar waveform <span class=\"math-tex\">\\(\\psi^{(4)}_{\\ell m}\\)</span></li>\n\t<li>Metric multipolar waveform <span class=\"math-tex\">\\(h_{\\ell m}\\)</span></li>\n\t<li>Radiated energy and angular momentum</li>\n</ul>\n\n<p>Files:</p>\n\n<ul>\n\t<li><em>waveforms/Psi4_l?_m?_r200.txt </em>\n\n\t<ul>\n\t\t<li>Columns: <span class=\"math-tex\">\\(t,\\ \\Re{(\\psi^{(4)}_{\\ell m})},\\ \\Im{(\\psi^{(4)}_{\\ell m})} \\)</span></li>\n\t</ul>\n\t</li>\n\t<li><em>waveforms/Rh_l?_m?_r200.txt</em>\n\t<ul>\n\t\t<li>Columns: <span class=\"math-tex\">\\(u/M,\\ \\Re{(h_{\\ell m})}/M,\\ \\Im{(h_{\\ell m})}/M,\\ \\Re{(\\dot{h}_{\\ell m})},\\ \\Im{(\\dot{h}_{\\ell m}}),\\ M\\omega_{\\ell m},\\ A_{\\ell m}/M,\\ \\phi_{\\ell m},\\ t \\)</span></li>\n\t</ul>\n\t</li>\n\t<li><em>waveforms/Ej_r200.txt</em>\n\t<ul>\n\t\t<li>Columns: <span class=\"math-tex\">\\(E_b,\\ j,\\ E_\\text{rad},\\ J_\\text{rad},\\ t \\)</span></li>\n\t</ul>\n\t</li>\n</ul>\n\n<p>where</p>\n\n<ul>\n\t<li><span class=\"math-tex\">\\(t\\)</span> simulation time</li>\n\t<li><span class=\"math-tex\">\\(u\\)</span> retarded time</li>\n\t<li><span class=\"math-tex\">\\(M\\)</span> binary mass</li>\n\t<li><span class=\"math-tex\">\\(\\omega_{\\ell m}\\)</span> wave frequency</li>\n\t<li><span class=\"math-tex\">\\(A_{\\ell m}\\)</span> wave amplitude</li>\n\t<li><span class=\"math-tex\">\\(\\phi_{\\ell m}\\)</span> wave phase</li>\n\t<li><span class=\"math-tex\">\\(E_\\text{GW}\\)</span> radiated energy</li>\n\t<li><span class=\"math-tex\">\\(J_\\text{GW}\\)</span> radiated angular momentum</li>\n\t<li><span class=\"math-tex\">\\(E_b\\)</span> binary energy</li>\n\t<li><span class=\"math-tex\">\\(j\\)</span> binary specific angular momentum</li>\n</ul>\n\n<p>Please refer to the paper and references therein for the definition of the different quantities.</p>\n\n<p>Units <span class=\"math-tex\">\\(c=G=M_\\text{Sun}=1\\)</span></p>", 
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  "identifier": "https://doi.org/10.5281/zenodo.57844", 
  "keywords": [
    "Binary neutron stars", 
    "Gravitational waves", 
    "Numerical relativity"
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  "license": "http://creativecommons.org/publicdomain/zero/1.0/legalcode", 
  "name": "How loud are neutron star mergers?", 
  "url": "https://zenodo.org/record/57844"
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