Abstract
Abstract
We describe a procedure for locating black hole horizons in ‘Kerr–Schild’ spacetimes in the double copy paradigm. Using only single- and zeroth-copy data on flat spacetime, our procedure predicts the existence of trapped surfaces in the double-copy gravitational solution. We show explicitly how this procedure locates the horizon of the Schwarzschild black hole and the general Myers–Perry black hole.
Funder
U.S. Department of Energy
Heising-Simons Foundation
Subject
Physics and Astronomy (miscellaneous)
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