Bulletin of the American Physical Society
APS April Meeting 2019
Volume 64, Number 3
Saturday–Tuesday, April 13–16, 2019; Denver, Colorado
Session H17: WIMP Dark Matter II
10:45 AM–12:33 PM,
Sunday, April 14, 2019
Sheraton
Room: Grand Ballroom II
Sponsoring
Unit:
DPF
Chair: Ben Loer, Pacific Northwest National Laboratory
Abstract: H17.00005 : Projected Performance of Future Liquid Xenon Detectors*
11:33 AM–11:45 AM
View Presentation
Abstract
Presenter:
Vetri Velan
(University of California, Berkeley)
Author:
Vetri Velan
(University of California, Berkeley)
Collaboration:
Large Underground Xenon (LUX)
The two-phase liquid xenon time projection chamber is one of the leading technologies used for dark matter direct detection. World-leading limits on dark matter interactions have been set by LUX and XENON1T, and the upcoming LZ and XENONnT experiments seek to push further. A crucial part of using this technology is being able to classify energy deposits as nuclear recoils (NR) or electron recoils (ER). In my talk, I will discuss how ER-NR discrimination can influence the performance of future detectors, informed by our analysis of LUX calibration data. I will focus on this via two paradigms: effects on discrimination from detector parameters like electric field and light collection, and from physical variables like pulse-shape and energy. Then, I will show the direct effects of discrimination on experiments' sensitivities to dark matter models.
*I am supported by the Graduate Instrumentation Research Award, established by CPAD and funded by the DOE. (This fellowship was awarded for a different project which I am not presenting at APS.)
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