XENONnT WIMP search: signal and background modeling and statistical inference

The XENONnT experiment searches for weakly interacting massive particle (WIMP) dark matter scattering off a xenon nucleus. In particular, XENONnT uses a dual-phase time projection chamber with a 5.9-ton liquid xenon target, detecting both scintillation and ionization signals to reconstruct the energ...

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Main Authors: Aprile, Elena (Author) , Lindner, Manfred (Author) , Marrodán Undagoitia, Teresa (Author) , Terliuk, Andrii (Author)
Format: Article (Journal)
Language:English
Published: 19 May, 2025
In: Physical review
Year: 2025, Volume: 111, Issue: 10, Pages: 1-21
ISSN:2470-0029
DOI:10.1103/PhysRevD.111.103040
Online Access:Verlag, kostenfrei, Volltext: https://doi.org/10.1103/PhysRevD.111.103040
Verlag, kostenfrei, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.111.103040
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Author Notes:XENON Collaboration*
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Summary:The XENONnT experiment searches for weakly interacting massive particle (WIMP) dark matter scattering off a xenon nucleus. In particular, XENONnT uses a dual-phase time projection chamber with a 5.9-ton liquid xenon target, detecting both scintillation and ionization signals to reconstruct the energy, position, and type of recoil. A blind search for nuclear recoil WIMPs with an exposure of 1.1 ton-years (4.18 t fiducial mass) yielded no signal excess over background expectations, from which competitive exclusion limits were derived on WIMP-nucleon elastic scatter cross sections, for WIMP masses ranging from 6 GeV/𝑐2 up to the TeV/𝑐2 scale. This work details the modeling and statistical methods employed in this search. By means of calibration data, we model the detector response, which is then used to derive background and signal models. The construction and validation of these models is discussed, alongside additional purely data-driven backgrounds. We also describe the statistical inference framework, including the definition of the likelihood function and the construction of confidence intervals.
Item Description:Veröffentlicht: 19. Mai 2025
XENON Collaboration: E. Aprile, M. Lindner, T. Marrodán Undagoitia, A. Terliuk [und 159 weitere Personen]
Gesehen am 29.10.2025
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Physical Description:Online Resource
ISSN:2470-0029
DOI:10.1103/PhysRevD.111.103040