Vacuum polarization on three-dimensional anti-de Sitter space-time with Robin boundary conditions
Sivakumar Namasivayam, Elizabeth Winstanley

TL;DR
This paper analyzes the vacuum polarization of a quantum scalar field in three-dimensional anti-de Sitter space with various boundary conditions, revealing how Robin conditions affect the expectation values and their dependence on space-time location.
Contribution
It provides a detailed study of vacuum and thermal expectation values of scalar fields in AdS3 with Robin boundary conditions, highlighting their dependence on boundary parameters and space-time location.
Findings
Finite vacuum polarization for Robin boundary conditions below a critical parameter
Constant expectation values for Neumann and Dirichlet boundary conditions
Robin boundary conditions lead to location-dependent expectation values
Abstract
We study a quantum scalar field, with general mass and coupling to the scalar curvature, propagating on three-dimensional global anti-de Sitter space-time. We determine the vacuum and thermal expectation values of the square of the field, also known as the vacuum polarisation (VP). We consider values of the scalar field mass and coupling for which there is a choice of boundary conditions giving well-posed classical dynamics. We apply Dirichlet, Neumann and Robin (mixed) boundary conditions to the field at the space-time boundary. We find finite values of the VP when the parameter governing the Robin boundary conditions is below a certain critical value. For all couplings, the vacuum expectation values of the VP with either Neumann or Dirichlet boundary conditions are constant and respect the maximal symmetry of the background space-time. However, this is not the case for Robin boundary…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Quantum Electrodynamics and Casimir Effect · Noncommutative and Quantum Gravity Theories
