Polluting the pair-instability mass gap for binary black holes through super-Eddington accretion in isolated binaries

<p>These are the results from:</p> <p>&quot;Polluting the pair-instability mass gap for binary black holes through super-Eddington accretion in isolated binaries&quot;<br> Authors: L.A.C. van Son, S. E. de Mink, F. S. Broekgaarden, M. Renzo, S. Justham, E. Laplace, J. Moran-Fraile, D. D. Hendriks, and R. Farmer</p> <p>ADS: &nbsp;&nbsp; &nbsp;https://ui.adsabs.harvard.edu/abs/2020arXiv200405187V/abstract<br> arXiv:&nbsp;&nbsp; &nbsp;https://arxiv.org/abs/2004.05187</p> <p>If you use (part of) these results in a scientific publication, we would greatly appreciate it if you would cite the source paper.</p> <p>This work uses <a href="https://compas.science/">COMPAS</a> to compute binary population properties (<a href="http://https://github.com/TeamCOMPAS/COMPAS/tree/master/docs">https://github.com/TeamCOMPAS/COMPAS/tree/master/docs</a>).</p> <p>*****************************</p> <p>For each of our 4 model variations (0. Fiducial, 1. Stable accretion, 2. Common envelope accretion and 3. Combined) we provide 2 files:</p> <p>1.) pythonSubmit.py file describing the initial conditions that were used to run the simulations</p> <p>2.) COMPASOutput.h5 file, which contains the following datasets resulting from our simulations :<br> [&#39;systems&#39;,<br> &nbsp;&#39;doubleCompactObjects&#39;,<br> &nbsp;&#39;commonEnvelopes&#39;,<br> &nbsp;]</p> <p>Detailed descriptions of these groups can be found in the accompanying README file.</p>