
A hypothetical very light particle that could explain certain cosmological observations, such as CMB polarization rotation.An ultralight axion is a hypothetical elementary particle with a mass far smaller than that of an electron, often in the range of 10^-22 to 10^-10 eV/c². It is a leading candidate for dark matter, the invisible substance that makes up about 27% of the universe. Ultralight axions are predicted to have a very long de Broglie wavelength, meaning they behave more like waves than particles on galactic scales, potentially explaining certain cosmological observations such as the rotation of the polarization plane of cosmic microwave background (CMB) radiation.
The axion was first proposed in 1977 by Roberto Peccei and Helen Quinn to solve the strong CP problem in particle physics, and later realized to be a dark matter candidate. The idea of ultralight axions (also called fuzzy dark matter) was developed in the 2000s by Wayne Hu, Rennan Barkana, and Andrei Gruzinov.
Axions interact with photons through a coupling that causes the polarization of light to rotate as it travels through an axion background. This effect, known as cosmic birefringence, would leave a distinct signature in the CMB polarization pattern. The axion field oscillates coherently, and its interaction with electromagnetic fields is described by a term in the Lagrangian that couples the axion field to the electromagnetic field tensor. The rotation angle depends on the axion mass and coupling strength, allowing observations to constrain these parameters.
Currently used in experimental searches for dark matter, such as the Axion Dark Matter Experiment (ADMX), which looks for axion-photon conversion in a microwave cavity.
If ultralight axions exist, they would form a coherent wave that could create interference patterns in the Milky Way's dark matter halo, potentially detectable as tiny oscillations in pulsar timing.








