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Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX data
LUX Collaboration, D. S. Akerib, H. M. Araújo +99
We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including $1.4\ti…
First results from the LUX dark matter experiment at the Sanford Underground Research Facility
LUX Collaboration, D. S. Akerib, H. M. Araujo +100
The Large Underground Xenon (LUX) experiment, a dual-phase xenon time-projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), was cooled and…
The Luminous Convolution Model
S. Cisneros, N. S. Oblath, J. A. Formaggio +5
We present a heuristic model for predicting the rotation curves of spiral galaxies. The Luminous Convolution Model (LCM) utilizes Lorentz-type transformations of very small changes…