Abstract
In this paper, we investigate the holographic complexity growth rate of the AdS accelerating black hole with a small mass for Einstein gravity by using the “complexity equals action” (CA-duality). By considering the contributions from the bulk, boundary term, and joint terms, we find the result of the action growth at the late time. In particular, we find the action growth only relies on the conical deficits parameter K and is independent of the accelerating A.
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