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M

M. Horn

Researcher at Yale University

Publications -  20
Citations -  2988

M. Horn is an academic researcher from Yale University. The author has contributed to research in topics: Dark matter & WIMP. The author has an hindex of 10, co-authored 15 publications receiving 2756 citations. Previous affiliations of M. Horn include Imperial College London.

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Journal ArticleDOI

First results from the LUX dark matter experiment at the Sanford Underground Research Facility

D. S. Akerib, +101 more
TL;DR: The first WIMP search data set is reported, taken during the period from April to August 2013, presenting the analysis of 85.3 live days of data, finding that the LUX data are in disagreement with low-mass W IMP signal interpretations of the results from several recent direct detection experiments.
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.
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.

First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment

Jelle Aalbers, +340 more
TL;DR: Results from LZ’s first search for Weakly Interacting Massive Particles with an exposure of 60 live days are reported, setting new limits on spin-independent WIMp-nucleon cross-sections for WIMP masses above 9 GeV / c 2.
Journal ArticleDOI

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

D. S. Akerib, +81 more
TL;DR: In this paper, the expected background rate from the background model for the 85.3-day WIMP search run is (2.6 ± 0.4 stat ) × 10 - 3 events keV ee - 1 kg - 1 day - 1, consistent with model projections.