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A. Currie

Researcher at Imperial College London

Publications -  16
Citations -  3100

A. Currie is an academic researcher from Imperial College London. The author has contributed to research in topics: Dark matter & ZEPLIN-III. The author has an hindex of 11, co-authored 16 publications receiving 2794 citations.

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Journal ArticleDOI

Results from a Search for Dark Matter in the Complete LUX Exposure

D. S. Akerib, +100 more
TL;DR: This search yields no evidence of WIMP nuclear recoils and constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35×10^{4} kg day exposure of the Large Underground Xenon experiment are reported.
Journal ArticleDOI

Improved limits on scattering of weakly interacting massive particles from reanalysis of 2013 LUX data

D. S. Akerib, +100 more
TL;DR: This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV.
ReportDOI

LUX-ZEPLIN (LZ) Conceptual Design Report

D. S. Akerib, +194 more
TL;DR: The design and performance of the LUX-ZEPLIN (LZ) detector is described as of March 2015 in this Conceptual Design Report as mentioned in this paper. And the LZ detector will be located at the Sanford Underground Research Facility in South Dakota.
Journal ArticleDOI

Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment.

D. S. Akerib, +100 more
TL;DR: The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.
Posted Content

After LUX: The LZ Program

D.C. Malling, +73 more
TL;DR: 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 is a 20-tonne detector as mentioned in this paper, which will probe spin-independent interaction cross sections as low as 5E-49 cm2 for 100 GeV WIMPs.