Abstract
In a Friedmann–Robertson–Walker (FRW) cosmological model with zero spatial curvature, we consider the interaction of the gravitational waves with the plasma in the presence of a weak magnetic field. Using the relativistic hydromagnetic equations, it is verified that large-amplitude magnetosonic waves are excited, assuming that both the gravitational field and the weak magnetic field do not break the homogeneity and isotropy of the considered FRW spacetime.
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