Abstract

We study a real, massive Klein-Gordon field in the Poincar\'e fundamental domain of the $(d+1)$-dimensional anti-de Sitter (AdS) spacetime, subject to a particular choice of dynamical boundary conditions of generalized Wentzell type, whereby the boundary data solves a non-homogeneous, boundary Klein-Gordon equation, with the source term fixed by the normal derivative of the scalar field at the boundary. This naturally defines a field in the conformal boundary of the Poincar\'e fundamental domain of AdS. We completely solve the equations for the bulk and boundary fields and investigate the existence of bound state solutions, motivated by the analogous problem with Robin boundary conditions, which are recovered as a limiting case. Finally, we argue that both Robin and generalized Wentzell boundary conditions are distinguished in the sense that they are invariant under the action of the isometry group of the AdS conformal boundary, a condition which ensures in addition that the total flux of energy across the boundary vanishes.

Highlights

  • Classical and quantum field theory on asymptotically anti–de Sitter (AdS) spacetimes, and generally other spacetimes with boundaries, has been the target of significant attention in the last two decades, mainly inspired by the remarkable AdS/CFT correspondence [1,2], see [3] for a modern overview

  • Massive Klein-Gordon field in the Poincarefundamental domain of the (d þ 1)dimensional anti–de Sitter (AdS) spacetime, subject to a particular choice of dynamical boundary conditions of generalized Wentzell type, whereby the boundary data solves a nonhomogeneous, boundary Klein-Gordon equation, with the source term fixed by the normal derivative of the scalar field at the boundary

  • We argue that both Robin and generalized Wentzell boundary conditions are distinguished in the sense that they are invariant under the action of the isometry group of the AdS conformal boundary, a condition which ensures in addition that the total flux of energy across the boundary vanishes

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Summary

INTRODUCTION

Classical and quantum field theory on asymptotically anti–de Sitter (AdS) spacetimes, and generally other spacetimes with boundaries, has been the target of significant attention in the last two decades, mainly inspired by the remarkable AdS/CFT correspondence [1,2], see [3] for a modern overview. By means of a Fourier transform, the Klein-Gordon equation has been reduced to a Sturm-Liouville problem, which naturally provides all the admissible boundary conditions of Robin type for a specific range of the mass parameter of the field In this context, studying all admissible Robin boundary conditions at once is a good strategy for finding the parameter space in mass and curvature coupling for which there exist bound state solutions, which decay exponentially away from the AdS boundary. As we shall see below, these boundary conditions have boundary data determined by a non-homogeneous, boundary KleinGordon equation, with the source term fixed by the normal derivative of the scalar field at the boundary This naturally defines a field in the conformal boundary of the Poincarefundamental domain of AdS, a feature which is clearly reminiscent of the AdS/CFT framework, though here we limit ourselves to considering noninteracting models. Throughout the paper we employ natural units in which c 1⁄4 GN 1⁄4 1 and a metric with signature (−þþ Á Á Á)

Geometry of anti–de Sitter spacetime
WENTZELL BOUNDARY CONDITIONS
Action
Regular case
Bulk and boundary solutions
Existence of bound states
Robin boundary conditions
Singular case
Vanishing symplectic and energy flux across the boundary
Interplay between the boundary conditions and the boundary isometry group
CONCLUSIONS
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