Gravitational Wave Backreaction in $f(R,G)$ Gravity

Abstract

We present a comprehensive theoretical framework for gravitational wave (GW) propagation and their \textbf{nonlinear backreaction} in $f(R, G)$ modified gravity. By developing a scalar-tensor formulation with two auxiliary fields, we systematically investigate both the propagation and backreaction of high-frequency gravitational waves in cosmological backgrounds. Within this framework, we derive, for the first time, the complete effective energy-momentum tensor for GWs in $f(R, G)$ theory. The linearized field equations reveal how the Gauss-Bonnet term introduces new curvature-dependent couplings between tensor and scalar degrees of freedom, leading to modified dispersion relations and distinctive wave propagation effects. On de Sitter backgrounds, we obtain exact decoupled equations for the tensor and scalar modes, demonstrating how the additional $G$ dependence alters both the effective masses and energy transport mechanisms compared to the well-established framework of pure $f(R)$ theories. Our derivation of the effective energy-momentum tensor extends Isaacson's approach to incorporate the novel scalar field contributions, revealing a complex hierarchy of characteristic length scales ($λ$, $\ell$, and $\mathcal{L}$) that govern the backreaction dynamics. The resulting formalism suggests potentially observable signatures in both the propagation (phase shifts, amplitude modulation) and stochastic background of gravitational waves. These effects could be probed by next-generation detectors, offering new constraints on the $f(R, G)$ coupling parameters. The theoretical framework developed here provides a foundation for future studies of gravitational wave generation in modified gravity scenarios and their role in the formation of cosmological structures.