Measurements and models of enhanced recombination following inner-shell vacancies in liquid xenon

Electron-capture decays of Xe125 and Xe127, and double-electron-capture decays of Xe124, are backgrounds in searches for weakly interacting massive particles (WIMPs) conducted by dual-phase xenon time projection chambers such as LUX-ZEPLIN (LZ). These decays produce signals with more light and less charge than equivalent-energy β decays and correspondingly overlap more with WIMP signals. We measure three electron-capture charge yields in LZ: the 1.1 keV M-shell, 5.2 keV L-shell, and 33.2 keV K-shell at drift fields of 193 and 96.5 V/cm. The LL double-electron-capture decay of Xe124 exhibits even more pronounced shifts in charge and light. We provide a first model of double-electron-capture charge yields using the link between ionization density and electron-ion recombination, and identify a need for more accurate calculations. Finally, we discuss the implications of the reduced charge yield of these decays and other interactions creating inner-shell vacancies for future dark matter searches.

Publication Details

Journal
Universität Zürich, ZORA
Published
2025-07-30
DOI
https://doi.org/10.5167/uzh-282355
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
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article

Measurements and models of enhanced recombination following inner-shell vacancies in liquid xenon

Universität Zürich, ZORA
Dark Matter and Cosmic Phenomena
article

Measurements and models of enhanced recombination following inner-shell vacancies in liquid xenon

article en

Abstract

Electron-capture decays of Xe125 and Xe127, and double-electron-capture decays of Xe124, are backgrounds in searches for weakly interacting massive particles (WIMPs) conducted by dual-phase xenon time projection chambers such as LUX-ZEPLIN (LZ). These decays produce signals with more light and less charge than equivalent-energy β decays and correspondingly overlap more with WIMP signals. We measure three electron-capture charge yields in LZ: the 1.1 keV M-shell, 5.2 keV L-shell, and 33.2 keV K-shell at drift fields of 193 and 96.5 V/cm. The LL double-electron-capture decay of Xe124 exhibits even more pronounced shifts in charge and light. We provide a first model of double-electron-capture charge yields using the link between ionization density and electron-ion recombination, and identify a need for more accurate calculations. Finally, we discuss the implications of the reduced charge yield of these decays and other interactions creating inner-shell vacancies for future dark matter searches.

Universität Zürich, ZORA
Openalex Percentile: Top 20%
Dark Matter and Cosmic Phenomena
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