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Self-adjoint wave equations for dynamical perturbations of self-gravitating fields

O. Sarbach·M. Heusler·O. Brodbeck
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Abstract

It is shown that the dynamical evolution of linear perturbations on a static space-time is governed by a constrained wave equation for the extrinsic curvature tensor. The spatial part of the wave operator is manifestly elliptic and self-adjoint. In contrast to metric formulations, the curvature-based approach to gravitational perturbation theory generalizes in a natural way to self-gravitating matter fields. It is also demonstrated how to obtain symmetric pulsation equations for self-gravitating non-Abelian gauge fields, Higgs fields and perfect fluids. For vacuum fluctuations on a vacuum space-time, the Regge-Wheeler and Zerilli equations are rederived.

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O. Sarbach, M. Heusler, O. Brodbeck. 2000-10-19. Self-adjoint wave equations for dynamical perturbations of self-gravitating fields. https://doi.org/10.1103/physrevd.63.104015

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