We study out-of-time-order correlators (OTOCs) of rotating BTZ black holes using two different approaches: the elastic eikonal gravity approximation, and the Chern-Simons formulations of 3-dimensional gravity. Within both methods the OTOC is given as a sum of two contributions, corresponding to left and right moving modes. The contributions have different Lyapunov exponents, λ ± L = 2π β 1 1∓ Ω , where Ω is the angular velocity and is the AdS radius. Since λ − L ≤ 2π β ≤ λ + L , there is an apparent contradiction with the chaos bound. We discuss how the result can be made consistent with the chaos bound if one views the parameters β ± = β(1 ∓ Ω) as the effective inverse temperatures of the left and right moving modes.
arXiv:1903.09086v2 [hep-th] 12 Apr 2019Contents 1 These recent developments were reviewed in [4,5].