Gravitomagnetic amplification in cosmology

Christos G. Tsagas
Phys. Rev. D 81, 043501 – Published 1 February 2010

Abstract

Magnetic fields interact with gravitational waves in various ways. We consider the coupling between the Weyl and the Maxwell fields in cosmology and study the effects of the former on the latter. The approach is fully analytical and the results are gauge invariant. We show that the nature and the outcome of the gravitomagnetic interaction depends on the electric properties of the cosmic medium. When the conductivity is high, gravitational waves reduce the standard (adiabatic) decay rate of the B field, leading to its superadiabatic amplification. In poorly conductive environments, on the other hand, Weyl-curvature distortions can result into the resonant amplification of large-scale cosmological magnetic fields. Driven by the gravitational waves, these B fields oscillate with an amplitude that is found to diverge when the wavelengths of the two sources coincide. We present technical and physical aspects of the gravitomagnetic interaction and discuss its potential implications.

  • Received 16 December 2009

DOI:https://doi.org/10.1103/PhysRevD.81.043501

©2010 American Physical Society

Authors & Affiliations

Christos G. Tsagas

  • Section of Astrophysics, Astronomy and Mechanics, Department of Physics, Aristotle University of Thessaloniki, Thessaloniki 54124, Greece

See Also

Gravitoelectromagnetic resonances

Christos G. Tsagas
Phys. Rev. D 84, 043524 (2011)

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Vol. 81, Iss. 4 — 15 February 2010

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