Modeling Flows Around Merging Black Hole Binaries

@article{Meter2010ModelingFA,
  title={Modeling Flows Around Merging Black Hole Binaries},
  author={James R. van Meter and John H. Wise and M. Coleman Miller and Christopher S. Reynolds and Joan M. Centrella and John G. Baker and William D. Boggs and Bernard J. Kelly and S. T. McWilliams},
  journal={The Astrophysical Journal},
  year={2010},
  volume={711}
}
Coalescing massive black hole binaries are produced by the mergers of galaxies. The final stages of the black hole coalescence produce strong gravitational radiation that can be detected by the space-borne Laser Interferometer Space Antenna. In cases where the black hole merger takes place in the presence of gas and magnetic fields, various types of electromagnetic signals may also be produced. Modeling such electromagnetic counterparts of the final merger requires evolving the behavior of both… Expand

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