Simulation studies of the LUX ZEPLIN (LZ) detector calibrations and data analysis

Lead Research Organisation: University of Oxford
Department Name: Oxford Physics

Abstract

LUX-ZEPLIN is a next generation Dark Matter experiment to be deployed at the Sanford Underground Research facility in Lead, South Dakota (USA). It will use 10 tonnes of liquid xenon and 500 photomultiplier tubes (PMT) to detect extremely rare events of dark matter interactions with regular matter. For the unambiguous detection of the elusive dark matter particle called Weakly Interacting Massive Particle (WIMP) a rigorous detector calibration programme is required. The experiment will use a suite of internally dispersed (83mKr, 131Xe, 220Rn and CH4 labelled tritium) and externally deployed sealed neutron (AmLi, 205, 206BiBe, 252Cf, 88YeBe) and gamma (57Co, 22Na, 133Ba, 228Th) radiation sources to provide high statistics calibration of the response to background events and WIMP signal. Rare-event experiments require exquisitely a well-calibrated detector as well as extremely accurate simulations tuned on existing calibration data, to model the detector response. In addition to the calibrations, all data analysis steps have to be extremely robust. A very important step is to extract and identify single photons from the pulse trains that the digitizers record from the electronics chain comprising PMT, cabling, amplifier board and further cabling. Algorithms to do this exist and have been tested at a level suitable for existing experiments, however, further improvements can be made by incorporating new techniques and the expanded understanding of detail of the detector response. The goal of this project is to perform detailed simulations to provide an optimal understanding of the detector response to calibration sources. The project objective is to simulate events from neutron and gamma sources used in the LZ experiment and reconstruct events' position and energy spectra, which is a key part of the detector calibration. Improving on photon detection, reconstruction and triggering effort will involve generating simulations of particular events in a xenon time projection chamber (re-using calibration events, for example), events from data recorded in previous experiments and using all possible information that is available in order to provide and validate a suitably enhanced algorithms. The project is computer based, using GEANT-based simulation, the ROOT data analysis package and the LZAp analysis framework. It is carried out within the LZ Collaboration of which Oxford is a member. The particular project will also have an element of collaboration with our LZ colleagues at RAL who have responsibility for contributing to the LZ calibrations effort.

Publications

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Studentship Projects

Project Reference Relationship Related To Start End Student Name
ST/R505006/1 01/10/2017 30/09/2021
1935504 Studentship ST/R505006/1 01/10/2017 30/09/2021 Andrew Stevens
 
Description Outreach activities 
Form Of Engagement Activity Participation in an activity, workshop or similar
Part Of Official Scheme? No
Geographic Reach Local
Primary Audience Other audiences
Results and Impact Various activities as part of Oxford Physics outreach including Stargazing, nad stalls in the Oxford University Museums. COntent is mainly bringing article physics to the general public.
Year(s) Of Engagement Activity 2019,2020
URL https://www2.physics.ox.ac.uk/news/2020/02/04/stargazing-2020