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Published 2022 | Version v1
Journal article

An approximate likelihood for nuclear recoil searches with XENON1T data

  • 1. Physics Department, Columbia University, New York, NY (United States)
  • 2. Kamioka Observatory, Institute for Cosmic Ray Research, and Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Higashi-Mozumi, Hida, Gifu (Japan)
  • 3. INFN-Bologna (Italy)
  • 4. Department of Physics and Astronomy, University of Bologna (Italy)

Description

The XENON collaboration has published stringent limits on specific dark matter - nucleon recoil spectra from dark matter recoiling on the liquid xenon detector target. In this paper, we present an approximate likelihood for the XENON1T 1 t-year nuclear recoil search applicable to any nuclear recoil spectrum. Alongside this paper, we publish data and code to compute upper limits using the method we present. The approximate likelihood is constructed in bins of reconstructed energy, profiled along the signal expectation in each bin. This approach can be used to compute an approximate likelihood and therefore most statistical results for any nuclear recoil spectrum. Computing approximate results with this method is approximately three orders of magnitude faster than the likelihood used in the original publications of XENON1T, where limits were set for specific families of recoil spectra. Using this same method, we include toy Monte Carlo simulation-derived binwise likelihoods for the upcoming XENONnT experiment that can similarly be used to assess the sensitivity to arbitrary nuclear recoil signatures in its eventual 20 t-year exposure.

Availability note (English)

Available from: http://dx.doi.org/10.1140/epjc/s10052-022-10913-w

Additional details

Publishing Information

Journal Title
European Physical Journal. C, Particles and Fields (Online)
Journal Volume
82
Journal Issue
11
Journal Page Range
vp.
ISSN
1434-6052
CODEN
EPCFFB

Optional Information

Notes
AID: 989
Collaborations
XENON Collaboration