![]() ![]() Two-dimensional axisymmetric simulations with effective viscosity remain an efficient and informative way to model this late-time post-merger evolution. Gravitational Wave Physics and Astronomy Center, California State University Fullerton, Fullerton, CA 92834, United States of AmericaĬenter for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Physics and Astronomy, Northwestern University, Evanston, IL 60202, United States of Americaĭetectable electromagnetic counterparts to gravitational waves from compact binary mergers can be produced by outflows from the black hole-accretion disk remnant during the first 10 s after the merger. Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, D-14476 Potsdam, Germany TAPIR, Walter Burke Institute for Theoretical Physics, MC 350-17, California Institute of Technology, Pasadena, CA 91125, United States of AmericaĬornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14853, United States of America Department of Physics & Astronomy, Washington State University, Pullman, WA 99164, United States of Americaĭepartment of Physics & Astronomy, University of New Hampshire, 9 Library Way, Durham, NH 03824, United States of Americaĭepartment of Physics, University of Alberta, Edmonton, AB T6G 2E1, Canada
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