Generalization of the Regge-Wheeler Equation for Self-Gravitating Matter Fields
- 3 April 2000
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 84 (14) , 3033-3036
- https://doi.org/10.1103/physrevlett.84.3033
Abstract
It is shown that the dynamical evolution of perturbations on a static spacetime is governed by a standard pulsation equation for the extrinsic curvature tensor. The centerpiece of the pulsation equation is a wave operator whose spatial part is manifestly self-adjoint. In contrast to metric formulations, the curvature-based approach to perturbation theory generalizes in a natural way to self-gravitating matter fields, including non-Abelian gauge fields and perfect fluids. As an example, the pulsation equations for self-gravitating, non-Abelian gauge fields are explicitly shown to be symmetric.Keywords
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This publication has 16 references indexed in Scilit:
- All nonspherical perturbations of the Choptuik spacetime decayPhysical Review D, 1999
- Gravitational waves from pulsating stars: Evolving the perturbation equations for a relativistic starPhysical Review D, 1998
- Curvature-based gauge-invariant perturbation theory for gravity: A new paradigmPhysical Review D, 1998
- Axial Instability of Rotating Relativistic StarsThe Astrophysical Journal, 1998
- Rotating Solitons and Nonrotating, Nonstatic Black HolesPhysical Review Letters, 1997
- Stationary perturbations and infinitesimal rotations of static Einstein-Yang-Mills configurations with bosonic matterPhysical Review D, 1997
- Einstein and Yang-Mills Theories in Hyperbolic Form without Gauge FixingPhysical Review Letters, 1995
- Head-on collision of two black holes: Comparison of different approachesPhysical Review D, 1995
- Colliding black holes: The close limitPhysical Review Letters, 1994
- Universality and scaling in gravitational collapse of a massless scalar fieldPhysical Review Letters, 1993