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The Luminous Convolution Model as an alternative to dark matter in spiral galaxies
S. Cisneros, N. S. Oblath, J. A. Formaggio +6
The Luminous Convolution Model (LCM) demonstrates that it is possible to predict the rotation curves of spiral galaxies directly from estimates of the luminous matter. We consider…
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…
A Detailed Look at the First Results from the Large Underground Xenon (LUX) Dark Matter Experiment
M. Szydagis, D. S. Akerib, H. M. Araujo +77
LUX, the world's largest dual-phase xenon time-projection chamber, with a fiducial target mass of 118 kg and 10,091 kg-days of exposure thus far, is currently the most sensitive di…