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Constraining early dark energy with gravitational waves before recombination

Zachary J. Weiner1,*, Peter Adshead1,†, and John T. Giblin, Jr.2,3,‡

  • 1Illinois Center for Advanced Studies of the Universe & Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
  • 2Department of Physics, Kenyon College, Gambier, Ohio 43022, USA
  • 3CERCA/ISO, Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106, USA

  • *zweiner2@illinois.edu
  • †adshead@illinois.edu
  • ‡giblinj@kenyon.edu

Phys. Rev. D 103, L021301 – Published 12 January, 2021

DOI: https://doi.org/10.1103/PhysRevD.103.L021301

Abstract

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.

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