Magnetized gravitational waves
- 14 May 2001
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 63 (12) , 123507
- https://doi.org/10.1103/physrevd.63.123507
Abstract
We investigate the influence of cosmic magnetic fields on gravitational wave perturbations and find exact solutions on large scales. We show that a large-scale magnetic field can generate large-scale non-decaying gravitational waves. In the general case where gravitational waves are generated by other mechanisms, a large-scale magnetic field introduces a new decaying tensor mode and modifies the non-decaying mode. The direct effect of the magnetic field is to damp the gravitational waves, while an indirect magneto-curvature effect can either damp or boost the waves. A magnetic field also leads to a breaking of statistical isotropy, and the magnetic imprint on the tensor spectrum in principle provides a means of detecting a primordial field.Keywords
All Related Versions
This publication has 23 references indexed in Scilit:
- Nonlinear gravitational wave interactions with plasmasPhysical Review D, 2000
- Cosmological electromagnetic fields due to gravitational wave perturbationsPhysical Review D, 2000
- Cosmological magnetic fieldsPramana, 2000
- Gravitational wave experiments and early universe cosmologyPhysics Reports, 2000
- Radio Wave Emissions Due to Gravitational RadiationThe Astrophysical Journal, 2000
- Tensor microwave anisotropies from a stochastic magnetic fieldPhysical Review D, 2000
- Gravito-electromagnetismClassical and Quantum Gravity, 1998
- A gauge-invariant analysis of magnetic fields in general-relativistic cosmologyClassical and Quantum Gravity, 1997
- Detection of anisotropies in the gravitational-wave stochastic backgroundPhysical Review D, 1997
- Constraints on a Primordial Magnetic FieldPhysical Review Letters, 1997