English

Improving sensitivity to low-mass dark matter in LUX using a novel electrode background mitigation technique

High Energy Physics - Experiment 2021-07-28 v1 Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics Instrumentation and Detectors

Abstract

This paper presents a novel technique for mitigating electrode backgrounds that limit the sensitivity of searches for low-mass dark matter (DM) using xenon time projection chambers. In the LUX detector, signatures of low-mass DM interactions would be very low energy (\simkeV) scatters in the active target that ionize only a few xenon atoms and seldom produce detectable scintillation signals. In this regime, extra precaution is required to reject a complex set of low-energy electron backgrounds that have long been observed in this class of detector. Noticing backgrounds from the wire grid electrodes near the top and bottom of the active target are particularly pernicious, we develop a machine learning technique based on ionization pulse shape to identify and reject these events. We demonstrate the technique can improve Poisson limits on low-mass DM interactions by a factor of 22-77 with improvement depending heavily on the size of ionization signals. We use the technique on events in an effective 55 tonne\cdotday exposure from LUX's 2013 science operation to place strong limits on low-mass DM particles with masses in the range mχ0.15m_{\chi}\in0.15-1010 GeV. This machine learning technique is expected to be useful for near-future experiments, such as LZ and XENONnT, which hope to perform low-mass DM searches with the stringent background control necessary to make a discovery.

Keywords

Cite

@article{arxiv.2011.09602,
  title  = {Improving sensitivity to low-mass dark matter in LUX using a novel electrode background mitigation technique},
  author = {LUX Collaboration and D. S. Akerib and S. Alsum and H. M. Araújo and X. Bai and J. Balajthy and J. Bang and A. Baxter and E. P. Bernard and A. Bernstein and T. P. Biesiadzinski and E. M. Boulton and B. Boxer and P. Brás and S. Burdin and D. Byram and M. C. Carmona-Benitez and C. Chan and J. E. Cutter and L. de Viveiros and E. Druszkiewicz and A. Fan and S. Fiorucci and R. J. Gaitskell and C. Ghag and M. G. D. Gilchriese and C. Gwilliam and C. R. Hall and S. J. Haselschwardt and S. A. Hertel and D. P. Hogan and M. Horn and D. Q. Huang and C. M. Ignarra and R. G. Jacobsen and O. Jahangir and W. Ji and K. Kamdin and K. Kazkaz and D. Khaitan and E. V. Korolkova and S. Kravitz and V. A. Kudryavtsev and E. Leason and B. G. Lenardo and K. T. Lesko and J. Liao and J. Lin and A. Lindote and M. I. Lopes and A. Manalaysay and R. L. Mannino and N. Marangou and D. N. McKinsey and D. -M. Mei and J. A. Morad and A. St. J. Murphy and A. Naylor and C. Nehrkorn and H. N. Nelson and F. Neves and A. Nilima and K. C. Oliver-Mallory and K. J. Palladino and C. Rhyne and Q. Riffard and G. R. C. Rischbieter and P. Rossiter and S. Shaw and T. A. Shutt and C. Silva and M. Solmaz and V. N. Solovov and P. Sorensen and T. J. Sumner and N. Swanson and M. Szydagis and D. J. Taylor and R. Taylor and W. C. Taylor and B. P. Tennyson and P. A. Terman and D. R. Tiedt and W. H. To and L. Tvrznikova and U. Utku and A. Vacheret and A. Vaitkus and V. Velan and R. C. Webb and J. T. White and T. J. Whitis and M. S. Witherell and F. L. H. Wolfs and D. Woodward and X. Xiang and J. Xu and C. Zhang},
  journal= {arXiv preprint arXiv:2011.09602},
  year   = {2021}
}

Comments

14 pages, 13 figures

R2 v1 2026-06-23T20:21:37.683Z