An action for reaction in general dimension
arXiv:1311.3196 · doi:10.1103/PhysRevD.89.045003
Abstract
We present an effective field theory study of radiation and radiation reaction effects for scalar and electromagnetic fields in general spacetime dimensions. Our method unifies the treatment of outgoing radiation and its reaction force within a single action principle. Central ingredients are the field doubling method, which is the classical version of the closed time path formalism and allows a treatment of non-conservative effects within an action, action level matching of system and radiation zones, and the use of fields which are adapted to the enhanced symmetries of each zone. New results include compact expressions for radiative multipoles, radiation, and radiation reaction effective action in any spacetime dimension. We emphasize dimension-dependent features such as the difference between electric and magnetic multipoles in higher dimensions and the temporal non-locality nature of the effective action for odd spacetime dimensions, which is a reflection of indirect propagation ("tail effect") in the full theory. This work generalizes the method and results developed for 4 dimensions in [arXiv:1305.6930], and prepares the way for a treatment of the gravitational case.
2 figures. generalizes arXiv:1305.6930
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Cited by in corpus (14)
- The Effective Field Theorist's Approach to Gravitational Dynamics
- Effective Field Theories of Post-Newtonian Gravity: A comprehensive review
- Theory of post-Newtonian radiation and reaction
- Self-interaction in classical gauge theories and gravitation
- Gravitational radiation-reaction in arbitrary dimension
- Self-forces in arbitrary dimensions
- Synchrotron radiation in odd dimensions
- Foundations of the self-force problem in arbitrary dimensions
- Static Self-Forces in a Five-Dimensional Black Hole Spacetime
- Radiation reaction at the level of the action
- Gravitational radiation from a binary system in odd-dimensional spacetime
- Leakage of gravitational waves into an extra dimension in the DGP model
- Comments on initial conditions for the Abraham-Lorentz(-Dirac) equation
- Scalar Wave Tails in Even Dimensional Weakly Curved Static Newtonian Spacetimes