- Open Access
Cosmology of gravitational axions
Phys. Rev. D 114, 023529 – Published 13 July, 2026
DOI: https://doi.org/10.1103/yst4-cr4c
Abstract
We show how a mass term for gravitational axions (“gravi-axions”) with a Chern-Simons coupling to gravity can naturally arise due to nonperturbative contributions from Euclidean wormholes, breaking the continuous shift symmetry of the standard theory. The induced mass can be generated in a cosmologically relevant range to be the dark matter or dark energy of the universe for a reasonable and well-motivated range of the symmetry breaking scale. Upon generating the gravi-axion mass term, we discuss the cosmology of the theory. We find that the gravi-axion can be produced to be the dominant dark matter component via misalignment or gravitational particle production, and that in a different regime, the gravi-axion can act as dynamical dark energy. We discuss gravi-axion decay into gravitons as a potential observational window for this theory. Finally, we find that, for late-time, astrophysical compact objects, cosmologically relevant gravi-axions behave as minimally coupled, massive scalar fields.
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