Affiliation:
1. McGill University
2. The University of Chicago
3. Enrico Fermi Institute, The University of Chicago
4. University of Winnipeg
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.
Published by the American Physical Society
2024
Funder
Canada First Research Excellence Fund
Kavli Institute for Cosmological Physics, University of Chicago
University of Chicago
U.S. Department of Energy
Natural Sciences and Engineering Research Council of Canada
Publisher
American Physical Society (APS)