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A measurement of the mean electronic excitation energy of liquid xenon

Abstract:
Liquid xenon is a leader in rare-event physics searches. Accurate modeling of charge and light production is key for simulating signals and backgrounds in this medium. The signal- and background-production models in the Noble Element Simulation Technique (NEST) are presented. NEST is a simulation toolkit based on experimental data, fit using simple, empirical formulae for the average charge and light yields and their variations. NEST also simulates the final scintillation pulses and exhibits the correct energy resolution as a function of the particle type, the energy, and the electric fields. After vetting of NEST against raw data, with several specific examples pulled from XENON, ZEPLIN, LUX/LZ, and PandaX, we interpolate and extrapolate its models to draw new conclusions on the properties of future detectors (e.g., XLZD's), in terms of the best possible discrimination of electron(ic) recoil backgrounds from a potential nuclear recoil signal, especially WIMP dark matter. We discover that the oft-quoted value of 99.5% discrimination is overly conservative, demonstrating that another order of magnitude improvement (99.95% discrimination) can be achieved with a high photon detection efficiency (g1 ~ 15-20%) at reasonably achievable drift fields of 200-350 V/cm.Comment: 24 Pages, 6 Tables, 15 Figures, and 15 Equation
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1140/epjc/s10052-021-09834-x

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Role:
Author
ORCID:
0000-0003-4710-1768
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Role:
Author
ORCID:
0000-0002-4814-0788
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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0003-3954-7612


Publisher:
SpringerOpen
Journal:
The European Physical Journal C More from this journal
Volume:
81
Issue:
12
Article number:
1060
Publication date:
2021-12-01
DOI:
EISSN:
1434-6052
ISSN:
1434-6044


Language:
English
Pubs id:
2285182
Local pid:
pubs:2285182
Source identifiers:
W3214896270
Deposit date:
2025-09-02
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