http://arxiv.org/abs/1602.04963
We describe the methods and results of numerical simulations of coalescing black holes. The simulation in dynamical spacetime covers the inspiral, merger, and ringdown phases. We analyze the emission of gravitational waves and properties of a black hole being the merger product. We discuss the results in the context of astrophysical environment of black holes that exist in the Universe.
A. Janiuk and S. Charzynski
Wed, 17 Feb 16
15/55
Comments: 6 pages; talk presented at the XXXVII Polish Astronomical Society Meeting
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