Axion detection experiments hunt for dark matter particles using specific frequency ranges and dwarf galaxy observations.Axions are hypothetical elementary particles that are a leading candidate for dark matter, the invisible substance that makes up about 85% of the universe's mass. Unlike heavy particles like WIMPs, axions would be extremely light — perhaps a billionth of the electron's mass — and would behave more like waves than particles. Detecting them requires entirely new experimental strategies, often involving powerful magnetic fields and ultra-sensitive microwave cavities, because axions are predicted to convert into photons in the presence of a magnetic field. The search for axions is one of the most active and exciting frontiers in particle physics and cosmology.
The axion was first proposed in 1977 by Roberto Peccei and Helen Quinn to solve the strong CP problem in quantum chromodynamics, and later realized to be a dark matter candidate by Frank Wilczek and Steven Weinberg. The first experimental searches began in the 1980s.
Axion detection experiments, such as ADMX, use a resonant cavity immersed in a strong magnetic field. If axions from the galactic dark matter halo pass through the cavity, a tiny fraction can convert into microwave photons with an energy equal to the axion mass. The cavity is tuned to a specific frequency, and by scanning through frequencies, researchers hope to hit the resonance that reveals the axion's mass. Dwarf galaxy observations complement these lab searches: because dwarf galaxies are dark matter-dominated, their gamma-ray or radio emissions could reveal axion decay or conversion signals, providing astrophysical evidence.
Axion searches drive the development of ultra-sensitive microwave detectors and quantum-limited amplifiers, technologies that also benefit quantum computing and precision metrology.
The Earth itself can act as a gravitational lens for axions, focusing them from all directions and potentially boosting the signal in a detector — a concept explored in recent theoretical studies.
| l_osc | variable | Oscillation length — length metre |
| E_c | variable | Critical energy — energy joule |
| E_γ | variable | Photon energy — energy joule |
| B_perp | variable | Perpendicular magnetic field strength — magnetic field strength tesla |
| g_aγ | variable | Axion-photon coupling constant — coupling constant inverse gev |


















