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Runaway Gravitational Production of Dark Photons

Christian Capanelli1,*, Leah Jenks2,†, Edward W. Kolb3,‡, and Evan McDonough4,§

  • *Contact author: christian.capanelli@mail.mcgill.ca
  • †Contact author: ljenks@uchicago.edu
  • ‡Contact author: Rocky.Kolb@uchicago.edu
  • §Contact author: e.mcdonough@uwinnipeg.ca

Phys. Rev. Lett. 133, 061602 – Published 9 August, 2024

DOI: https://doi.org/10.1103/PhysRevLett.133.061602

Abstract

We demonstrate that gravitational particle production of a massive, Abelian, vector (Proca) field during inflation in the presence of nonminimal coupling to gravity may suffer from an instability which leads to runaway production of high-momentum modes. This is untenable unless there is some mechanism to regulate the runaway. We discuss the parameter space of the particle mass and nonminimal couplings where such a runaway occurs and possible ways to tame the runaway. We find that there is no obvious way to resolve the runaway in a UV completion or with kinetic mixing to the standard model.

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