Ultraviolet Structure of Real-time Gravitational Wave Linear Response in a Resonant Scalar Field
This paper utilizes the Schwinger-Keldysh formalism and adiabatic regularization to analyze the ultraviolet structure of real-time gravitational wave linear response in a resonant scalar field, identifying specific time-dependent divergences that require new local counterterms and revealing a renormalization mismatch with the tadpole stress tensor that is attributed to the off-shell nature of the background.