Abstract
Axion cosmology is reexamined taking into account the effect of kinetic pseudo-Nambu-Goldstone modes. When Peccei-Quinn (PQ) symmetry is broken by a chiral U(1) singlet, we find that the effect of the kinetic Nambu-Goldstone mode makes the axion dark matter untenable. When PQ symmetry is extended and is broken by two singlets, we find that axion cosmology works, but there are several differences from the axion cosmology studied in the literature. The differences are (1) an ordinary type of dark matter scaling of arising from a modulus field and not from the usual angular field, (2) the mass of the dark matter quantum in the ultralight range , (3) the emergence of dark energy with a present density of order , consistent with observations, (4) the presence of a long-range spin-dependent force, and (5) slow-roll inflation after PQ symmetry breaking when conformal coupling to gravity is introduced.
- Received 9 February 2022
- Accepted 22 April 2022
DOI:https://doi.org/10.1103/PhysRevD.105.103522
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
Published by the American Physical Society