Natural Phantom Dark Energy from a $\mathbb{Z}_N$--Axion
Abstract
We present a technically natural microscopic realization of apparent phantom dark energy based on an axion coupled to copies of two-flavor dark QCD related by a exchange symmetry. The symmetry exponentially suppresses the axion vacuum potential, naturally generating the dark-energy scale, while reheating into a single dark sector induces a controlled breaking of that simultaneously restores the physical axion periodicity, sets the dark-matter abundance, and drives the late-time dark-energy dynamics. The selected sector contains dark-pion dark matter, whose finite density initially traps the axion away from its vacuum minimum. As the Universe expands and the dark-pion density redshifts away, the axion is released and rolls on the reheating-induced vacuum potential, generating an effective phantom crossing without tuned cancellations. We identify a viable parameter region that simultaneously reproduces the observed dark-matter relic abundance and dark-energy scale, satisfies cosmological and astrophysical constraints, and qualitatively reproduces the DESI preference for an evolving dark-energy equation of state.
Cite
@article{arxiv.2607.06774,
title = {Natural Phantom Dark Energy from a $\mathbb{Z}_N$--Axion},
author = {Cédric Delaunay and Admir Greljo},
journal= {arXiv preprint arXiv:2607.06774},
year = {2026}
}
Comments
17 pages