It has been suggested that certain antiferromagnetic topological insulators contain axion
quasiparticles (AQs), and that such materials could be used to detect axion dark matter …

We discuss axion dark matter detection via two mechanisms: spontaneous decays and
resonant conversion in neutron star magnetospheres. For decays, we show that the …

We present first results from a dark photon dark matter search in the mass range from 44 to
52 μ eV (10.7–12.5 GHz) using a room-temperature dish antenna setup called GigaBREAD …

The next generation of ultralight dark matter (DM) direct detection experiments, which could
confirm sub-eV bosons as the dominant source of DM, will feature multiple detectors …

In the presence of a background magnetic field, axion dark matter induces an electric field
and can thus excite phonon-polaritons in suitable materials. We revisit the calculation of the …

We report the results of the search for dark photons with mass around 1.5 eV/c 2 using a
multilayer dielectric haloscope equipped with an affordable and commercially available …

A bstract In the presence of axion dark matter, fermion spins experience an “axion wind”
torque and an “axioelectric” force. We investigate new experimental probes of these effects …

The reciprocity approach is a powerful method to determine the expected signal power of
axion haloscopes in a model-independent way. Especially for open and broadband setups …

The oscillating light axion field is known as wave dark matter. We propose an LC (inductor-
capacitor)-resonance enhanced detection of the narrow band electric signals induced by the …

Axion haloscopes search for dark matter axions from the galactic halo, most commonly by
measuring a power excess sourced by the axion effective current density. Constraining …