activity
20022026
most citedDirect Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory

3k citations · 13k across the 112 of their papers we have counts for

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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…

astro-ph.IM2014★ 77 cited

A Global Analysis of Light and Charge Yields in Liquid Xenon

Brian Lenardo, Kareem Kazkaz, Aaron Manalaysay +2

We present an updated model of light and charge yields from nuclear recoils in liquid xenon with a simultaneously constrained parameter set. A global analysis is performed using me…

astro-ph.IM2014★ 87 cited

Radiogenic and Muon-Induced Backgrounds in the LUX Dark Matter Detector

D. S. Akerib, H. M. Araujo, X. Bai +77

The Large Underground Xenon (LUX) dark matter experiment aims to detect rare low-energy interactions from Weakly Interacting Massive Particles (WIMPs). The radiogenic backgrounds i…

astro-ph.IM2013★ 32 cited

First demonstration of a sub-keV electron recoil energy threshold in a liquid argon ionization chamber

S. Sangiorgio, T. H. Joshi, A. Bernstein +9

We describe the first demonstration of a sub-keV electron recoil energy threshold in a dual-phase liquid argon time projection chamber. This is an important step in an effort to de…

astro-ph.IM2012★ 62 cited

Technical Results from the Surface Run of the LUX Dark Matter Experiment

LUX Collaboration, D. S. Akerib, X. Bai +64

We present the results of the three-month above-ground commissioning run of the Large Underground Xenon (LUX) experiment at the Sanford Underground Research Facility located in Lea…

astro-ph.IM2011★ 58 cited

After LUX: The LZ Program

D. C. Malling, D. S. Akerib, H. M. Araujo +71

The LZ program consists of two stages of direct dark matter searches using liquid Xe detectors. The first stage will be a 1.5-3 tonne detector, while the last stage will be a 20 to…