We show that rapidly-spinning black holes can display turbulent gravitational behavior which is mediated by a new type of parametric instability. This instability transfers energy from higher temporal and azimuthal spatial frequencies to lower frequencies--- a phenomenon reminiscent of the inverse energy cascade displayed by 2+1-dimensional turbulent fluids. Our finding reveals a path towards gravitational turbulence for perturbations of rapidly-spinning black holes, and provides the first evidence for gravitational turbulence in an asymptotically flat spacetime. Interestingly, this finding predicts observable gravitational wave signatures from such phenomena in black hole binaries with high spins and gives a gravitational description of turbulence relevant to the fluid-gravity duality.
@article{arxiv.1402.4859,
title = {Turbulent Black Holes},
author = {Huan Yang and Aaron Zimmerman and Luis Lehner},
journal= {arXiv preprint arXiv:1402.4859},
year = {2015}
}
Comments
5+3 pages, 2 figures, corrected an error in the treatment of the driving mode; example and figures changed, discussion added