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An asymptotic expansion of the above metric can be realized by defining coordinate ρ such that dρ ρ = dr r √ f(r)

Asymptotic expansion of BTZ The rotating BTZ metric is given as, ds2 =−(r2−r2 +)(r2−r2 −) r2 dt2 + r2 (r2−r2 +)(r2−r2 −) dr2 +r2 ( dx− r+r− r2 dt )2 , (A1) where r+,r− are the radi

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Inhomogeneous Jacobi equation and Holographic subregion complexity

hep-th · 2019-07-26 · unverdicted · novelty 5.0

A variational perturbative method using the inhomogeneous Jacobi equation computes first-order changes in holographic subregion complexity for strip and disk subsystems under boosted black brane perturbations in AdS4, with the linear term vanishing for spherical subsystems.

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  • Inhomogeneous Jacobi equation and Holographic subregion complexity hep-th · 2019-07-26 · unverdicted · none · ref 7

    A variational perturbative method using the inhomogeneous Jacobi equation computes first-order changes in holographic subregion complexity for strip and disk subsystems under boosted black brane perturbations in AdS4, with the linear term vanishing for spherical subsystems.