Scalar field dynamics in a BTZ background with generic boundary conditions

TL;DR

This paper analyzes the dynamics of a massive scalar field in a BTZ black hole background, exploring how different boundary conditions affect the well-posedness and positivity of solutions, especially within a specific mass range.

Contribution

It introduces a systematic approach to classify boundary conditions for scalar fields in BTZ spacetime, revealing the existence of a family of physically consistent evolutions.

Findings

Scalar field dynamics are well-defined for a specific mass window with a family of boundary conditions.

Uniqueness of boundary conditions for non-negative mass squared.

Energy remains positive and conserved across all considered evolutions.

Abstract

The revisit the dynamics of a massive scalar field in a BTZ background taking into account the lack of global hyperbolicity of the spacetime. We approach this issue using the strategy of Ishibashi and Wald which finds a unique smooth solution as the causal evolution of initial data, each possible evolution corresponding to a positive self-adjoint extension of certain operator in a Hilbert space on the initial surface. Moreover, solutions obtained this way are the most general ones satisfying a few physically-sensible requirements. This procedure is intimately related to the choice of boundary conditions and the existence of bound states. We find that the scalar field dynamics in the (effective) mass window $-3/4\leq m_e^2\ell^2<0$ can be well-defined within a one-parametric family of distinct boundary conditions ($-3/4$ being the conformally-coupled case), while for $m_e^2\ell^2\geq 0$ the boundary condition is unique (only one self-adjoint extension is possible). It is argued that there is no sensible evolution possible for $m_e^2\ell^2<-1$, and also shown that in the range $m_e^2\ell^2 \in [-1,-3/4)$ there is a U$(1)$ family of allowed boundary conditions, however, the positivity of the self-adjoint extensions is only motivated but not proven. We focus mainly in describing the dynamics of such evolutions given the initial data and all possible boundary conditions, and in particular we show the energy is always positive and conserved.