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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…
Projected WIMP sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment
D. S. Akerib, C. W. Akerlof, S. K. Alsum +175
LUX-ZEPLIN (LZ) is a next generation dark matter direct detection experiment that will operate 4850 feet underground at the Sanford Underground Research Facility (SURF) in Lead, So…
Supernova Neutrino Detection in LZ
Dev Ashish Khaitan
In the first 10 seconds of a core-collapse supernova, almost all of its progenitor's gravitational potential, O(10~ergs), is carried away in the form of neutrinos. These neu…
Xenon Bubble Chambers for Direct Dark Matter Detection
C. Levy, S. Fallon, J. Genovesi +4
The search for dark matter is one of today's most exciting fields. As bigger detectors are being built to increase their sensitivity, background reduction is an ever more challengi…