Dark matter, a type of matter that does not emit, absorb, or reflect light, is predicted to account for most of the universe’s mass. While theoretical predictions hint at its abundance, detecting this elusive matter has so far proved to be very difficult, leaving its composition and origin a mystery.
One widely explored hypothesis is that dark matter consists of weakly interacting massive particles, or WIMPs for short. These particles are theorized to only interact with ordinary matter via gravity and potentially via weak nuclear forces.
The LUX-ZEPLIN (LZ) experiment is a large-scale research effort aimed at searching for signals associated with the presence of WIMPs using a sophisticated detector known as a dual-phase xenon time projection chamber. The researchers involved in the experiment recently published their most recent findings in a paper in Physical Review Letters, which places more stringent constraints on lighter dark matter particles that could have gained energy after colliding with cosmic rays.