activity
19992026
most citedDirect Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory

3k citations · 17.5k across the 112 of their papers we have counts for

collaborators
Showing 2021Show all

5 papers · 1 filter

physics.ins-det2021★ 2 cited

Design and production of the high voltage electrode grids and electron extraction region for the LZ dual-phase xenon time projection chamber

R. Linehan, R. L. Mannino, A. Fan +46

The dual-phase xenon time projection chamber (TPC) is a powerful tool for direct-detection experiments searching for WIMP dark matter, other dark matter models, and neutrinoless do…

physics.ins-det2021★ 12 cited

Projected sensitivity of the LUX-ZEPLIN (LZ) experiment to the two-neutrino and neutrinoless double beta decays of Xe

The LUX-ZEPLIN, Collaboration, : +194

The projected sensitivity of the LUX-ZEPLIN (LZ) experiment to two-neutrino and neutrinoless double beta decay of Xe is presented. LZ is a 10-tonne xenon time projection ch…

hep-ex2021★ 29 cited

Projected sensitivities of the LUX-ZEPLIN (LZ) experiment to new physics via low-energy electron recoils

The LZ Collaboration, D. S. Akerib, A. K. Al Musalhi +194

LUX-ZEPLIN (LZ) is a dark matter detector expected to obtain world-leading sensitivity to weakly interacting massive particles (WIMPs) interacting via nuclear recoils with a ~7-ton…

astro-ph.CO2021★ 15 cited

Constraints on Effective Field Theory Couplings Using 311.2 days of LUX Data

D. S. Akerib, S. Alsum, H. M. Araújo +94

We report here the results of an Effective Field Theory (EFT) WIMP search analysis using LUX data. We build upon previous LUX analyses by extending the search window to include nuc…

astro-ph.IM2021★ 8 cited

Enhancing the sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment to low energy signals

D. S. Akerib, A. K. Al Musalhi, S. K. Alsum +184

Two-phase xenon detectors, such as that at the core of the forthcoming LZ dark matter experiment, use photomultiplier tubes to sense the primary (S1) and secondary (S2) scintillati…