Dark matter direct detection (XENON)

Layer 1 — Physicsin the multi-messenger-astrophysics subtree

XENONnT 2023 limits on WIMP-nucleon cross-section sigma_SI < 2.6 x 10^-47 cm^2 at 30 GeV/c^2; LUX-ZEPLIN + DARWIN successors; null results constraining WIMP parameter-space.

Related concepts

Explore Dark matter direct detection (XENON) on the interactive knowledge graph →