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Toward a Theory of Gravitational Wave Turbulence

Published 24 Sep 2025 in gr-qc, astro-ph.HE, hep-th, and physics.plasm-ph | (2509.19769v1)

Abstract: General relativity describes the dynamics of gravitational waves, which can feature nonlinear interactions, such as those underlying turbulent processes. Theoretical and numerical explorations have demonstrated the existence of gravitational wave turbulence, of which a full and general mathematical description is currently not known. Here, we take essential steps towards such a theory. Leveraging a formulation exactly recasting general relativity as a set of nonlinear electrodynamics equations, we demonstrate that general relativity admits an Elsasser formulation -- the same type of equation underpinning magnetohydrodynamic turbulence. We further show that nonlinear interactions described by this equation are in part Alfv\'enic, linking gravitational wave turbulence to Alfv\'enic turbulence. Our work paves the way for a new understanding of nonlinear gravitational wave dynamics through insights from magnetohydrodynamics.

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