Constraining early dark energy with gravitational waves before recombination

We show that the nonperturbative decay of ultralight scalars into Abelian gauge bosons, recently proposed as a possible solution to the Hubble tension, produces a stochastic background of gravitational waves which is constrained by the cosmic microwave background. We simulate the full nonlinear dynamics of resonant dark photon production and the associated gravitational-wave production, finding the signals to exceed constraints for the entire parameter space we consider. Our findings suggest that gravitational-wave production from the decay of early dark energy may provide a unique probe of these models.

Automated summary

Simulation of the nonperturbative decay of ultralight scalars into Abelian gauge bosons reveals an excess of gravitational-wave signals beyond constraints across the entire parameter space under consideration, suggesting that gravitational-wave production from the decay of early dark energy may offer a unique probe of these models.