Probing the Scalar WIMP-Pion Coupling with the first LUX-ZEPLIN data
arXiv:2406.02441 · doi:10.1038/s42005-024-01774-8
Abstract
Weakly interacting massive particles (WIMPs) may interact with a virtual pion that is exchanged between nucleons. This interaction channel is important to consider in models where the spin-independent isoscalar channel is suppressed. Using data from the first science run of the LUX-ZEPLIN dark matter experiment, containing 60 live days of data in a 5.5~tonne fiducial mass of liquid xenon, we report the results on a search for WIMP-pion interactions. We observe no significant excess and set an upper limit of ~cm at a 90\% confidence level for a WIMP mass of 33~GeV/c for this interaction.
References in corpus (32)
- Local Kinematics and the Local Standard of Rest
- The Galaxy in Context: Structural, Kinematic and Integrated Properties
- The Shell Model as Unified View of Nuclear Structure
- A History of Dark Matter
- Rotation Curves of Spiral Galaxies
- First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
- The RAVE Survey: Constraining the Local Galactic Escape Speed
- Dark Matter Search Results from the PandaX-4T Commissioning Run
- First Dark Matter Search with Nuclear Recoils from the XENONnT Experiment
- Combined Analysis of all Three Phases of Solar Neutrino Data from the Sudbury Neutrino Observatory
- A new Generation of Standard Solar Models
- Dark matter and the early Universe: a review
- The LUX-ZEPLIN (LZ) Experiment
- Improved GRAVITY astrometric accuracy from modeling of optical aberrations
- An improved measurement of the 2νββ half-life of Xe-136 with EXO-200
- Simultaneous Precision Spectroscopy of , Be, and Solar Neutrinos with Borexino Phase-II
- First observation of two-neutrino double electron capture in Xe with XENON1T
- WIMP-nucleus scattering in chiral effective theory
- Analysis strategies for general spin-independent WIMP-nucleus scattering
- Nuclear structure aspects of spin-independent WIMP scattering off xenon
- Nuclear structure factors for general spin-independent WIMP-nucleus scattering
- The LUX-ZEPLIN (LZ) radioactivity and cleanliness control programs
- Light stops, blind spots, and isospin violation in the MSSM
- Constraints on dark matter-nucleon effective couplings in the presence of kinematically distinct halo substructures using the DEAP-3600 detector
- Simulations of Events for the LUX-ZEPLIN (LZ) Dark Matter Experiment
- Background Determination for the LUX-ZEPLIN (LZ) Dark Matter Experiment
- First results on the scalar WIMP-pion coupling, using the XENON1T experiment
- First Constraints on WIMP-Nucleon Effective Field Theory Couplings in an Extended Energy Region From LUX-ZEPLIN
- Measurement of the Gamma Ray Background in the Davis Cavern at the Sanford Underground Research Facility
- Discriminating WIMP-nucleus response functions in present and future XENON-like direct detection experiments
- Cosmogenic production of Ar in the context of the LUX-ZEPLIN experiment
- Snowmass2021 Cosmic Frontier Dark Matter Direct Detection to the Neutrino Fog