Self-consistent interaction of linear gravitational and electromagnetic waves in non-magnetized plasma
Deepen Garg, I. Y. Dodin

TL;DR
This paper develops a self-consistent framework for analyzing the interaction between linear gravitational and electromagnetic waves in non-magnetized plasma, revealing significant effects on the dispersion of certain modes.
Contribution
It introduces a novel Hamiltonian approach to describe gravito-electromagnetic wave interactions in inhomogeneous plasma without symmetry assumptions.
Findings
Transverse gravitational waves do not interact with plasma or EM modes in the geometric optics limit.
Longitudinal GEM modes with high refraction index exhibit strong gravitational-electromagnetic interplay.
The dispersion relation of the Jeans mode is notably influenced by electrostatic interactions.
Abstract
This paper explores the hybridization of linear metric perturbations with linear electromagnetic (EM) perturbations in non-magnetized plasma for a general background metric. The local wave properties are derived from first principles for inhomogeneous plasma, without assuming any symmetries of the background metric. First, we derive the effective (``oscillation-center'') Hamiltonian that governs the average dynamics of plasma particles in a prescribed quasimonochromatic wave that involves metric perturbations and EM fields simultaneously. Then, using this Hamiltonian, we derive the backreaction of plasma particles on the wave itself and obtain gauge-invariant equations that describe the resulting self-consistent gravito-electromagnetic (GEM) waves in a plasma. The transverse tensor modes of gravitational waves are found to have no interaction with the plasma and the EM modes in the…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Pulsars and Gravitational Waves Research
