Constrained field theories on spherically symmetric spacetimes with horizons
arXiv:1608.02696 · doi:10.1103/PhysRevD.95.045012
Abstract
We apply the Dirac-Bergmann algorithm for the analysis of constraints to gauge theories defined on spherically symmetric black hole backgrounds. We find that the constraints for a given theory are modified on such spacetimes through the presence of additional contributions from the horizon. As a concrete example, we consider the Maxwell field on a black hole background, and determine the role of the horizon contributions on the dynamics of the theory.
arXiv comment23 pp
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