Abstract

We derive the exact gravitational field of a relativistic particle localized on an AdSAdS 3-brane, with curvature radius ℓ\ell, in AdS5AdS_5 bulk with radius LL. The solution is a gravitational shock wave. We use it to explore the dynamics of locally localized tensor gravitons over a wide range of scales. At distances below LL the shock wave looks exactly like the 5D5D GRGR solution. Beyond LL the solution approximates very closely the shock wave in 4D AdSAdS space all the way out to distances ℓ3/L2\ell^3/L^2 along the brane. At distances between LL and ℓ\ell, the effective 4D graviton is a composite built of the ultralight mode and heavier gravitons, whereas between ℓ\ell and ℓ3/L2\ell^3/L^2 it is just the ultralight mode. Finally beyond ℓ3/L2\ell^3/L^2 the shock reveals a glimpse of the fifth dimension, since the ultralight mode wave function decays to zero at the rate inherited from the full 5D5D geometry. We obtain the precise bulk-side formula for the 4D Planck mass, defined as the coupling of the ultralight mode, in terms of the 5D5D Planck mass and the curvature radii. It includes higher-order corrections in L/ℓL/\ell, and reduces to the RS2 formula in the limit ℓ→∞\ell \to \infty. We discuss AdS/CFTAdS/CFT interpretation of these results, and argue that the spatial variation of the effective gravitational coupling read from the shock wave amplitude corresponds to RG running driven by quantum effects in the dual CFTCFT.

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