Nonlinear dynamics driving the conversion of gravitational and electromagnetic waves in cylindrically symmetric spacetime
Takashi Mishima, Shinya Tomizawa

TL;DR
This paper constructs exact solutions for cylindrically symmetric gravitational and electromagnetic waves in Einstein-Maxwell theory, revealing nonlinear mode conversions and wave amplification effects near the symmetry axis.
Contribution
It introduces a novel method using composite harmonic mapping to analyze wave conversions in Einstein-Maxwell systems with exact solutions.
Findings
Notable mode conversions occur near the symmetry axis.
Electromagnetic mode amplification factors range from 0.4 to 2.4.
Wave modes tend to revert to initial states away from the axis in certain cases.
Abstract
Using the ``composite harmonic mapping method," we construct exact solutions for cylindrically symmetric gravitational and electromagnetic waves within the Einstein-Maxwell system, focusing on the conversion dynamics between these types of waves. In this approach, we employs two types of geodesic surfaces in : (a) the complex line and (b) the totally real Lagrangian plane, applied to two different vacuum seed solutions: (i) a vacuum solution previously utilized in our studies and (ii) the solitonic vacuum solution constructed previously by Economou and Tsoubelis. We study three scenarios: case (a) with seeds (i) and (ii), and case (b) with seed (ii). In all cases (a) and (b), solutions demonstrate notable mode conversions near the symmetric axis. In case (a) with seed (i) or seed (ii), we show that any change in the occupancy of the gravitational or electromagnetic…
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Taxonomy
TopicsCosmology and Gravitation Theories · Pulsars and Gravitational Waves Research · Relativity and Gravitational Theory
