Non-linear effects for cylindrical gravitational two-soliton
Abstract
Using a cylindrical soliton solution to the four-dimensional vacuum Einstein equation, we study non-linear effects of gravitational waves such as Faraday rotation and time shift phenomenon. In the previous work, we analyzed the single-soliton solution constructed by the Pomeransky's improved inverse scattering method. In this work, we construct a new two-soliton solution with complex conjugate poles, by which we can avoid light-cone singularities unavoidable in a single soliton case. In particular, we compute amplitudes of such non-linear gravitational waves and time-dependence of the polarizations. Furthermore, we consider the time shift phenomenon for soliton waves, which means that a wave packet can propagate at slower velocity than light.
Cite
@article{arxiv.1502.06331,
title = {Non-linear effects for cylindrical gravitational two-soliton},
author = {Shinya Tomizawa and Takashi Mishima},
journal= {arXiv preprint arXiv:1502.06331},
year = {2015}
}
Comments
13 pages, 8 figures