Abstract

We find an effective action for gravitational interactions with scalars in AdS3AdS_3 to first order in GNG_N at the conformal boundary. This action can be understood as an action for the Brown-Henneaux modes and is given by the square-root product of right and left moving Schwarzian derivatives for conformal transformations of the boundary. We thus reproduce the result λL=2πβλ_L=\frac{2π}β for OTOC computed first in arXiv:1412.6087 for a Schwarzchild black hole in AdS3AdS_3. Applying the same procedure to rotating BTZ we find the Lyapunov index to be λL=2πβ+>2πβλ_L=\frac{2π}{β_+}>\frac{2π}β where β+=β(1−μL)β_+=β(1-μ_L), with μL=r−r+μ_L=\frac{r_-}{r_+} being the chemical potential for angular momentum. We thus comment on a possible modification to a part of the proof given in arXiv:1503.01409 to accommodate this result.

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