Dark Matter
Empirical evidence for the existence of non-luminous, dark matter, which interacts gravitationally with ordinary matter and radiation, has been discovered in scales ranging from galactic to cosmological.
Empirical evidence for the existence of non-luminous, dark matter, which interacts gravitationally with ordinary matter and radiation, has been discovered in scales ranging from galactic to cosmological.
We are developing a new technology, based on finding single crystal defects in a bulk, that arise from interactions of light dark matter and a nucleus. These defects are long lived and spectroscopically active, which makes them ideal for detection of nuclear interactions with a threshold of tens of eV.
XLZD: a future xenon observatory for dark matter and other rare interactions.
Leading Xenon Researchers unite to build next-generation Dark Matter Detector