Displacement memory effect near the horizon of black holes

Abstract

We study the displacement memory effect and its connection with the extended-BMS symmetries near the horizon of black holes. Considering the near-horizon asymptotic metrics, we show there is a permanent shift in the geodesic deviation vector relating two nearby timelike geodesics placed close to the horizon of black holes, upon the passage of gravitational waves. We also relate this memory effect with the asymptotic symmetries of the near-horizon metric. For black holes, the shift of the relative position of the detectors is shown to be induced by a combination of BMS generators near the horizon. Particularly for extreme black holes, the displacement memory effect near the horizon is quite similar to the same obtained in the far region.