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First Constraint on Atmospheric Millicharged Particles with the LUX-ZEPLIN Experiment

  • J. Aalbers
  • , D. S. Akerib
  • , A. K.Al Musalhi
  • , F. Alder
  • , C. S. Amarasinghe
  • , A. Ames
  • , T. J. Anderson
  • , N. Angelides
  • , H. M. Araújo
  • , J. E. Armstrong
  • , M. Arthurs
  • , A. Baker
  • , S. Balashov
  • , J. Bang
  • , J. W. Bargemann
  • , E. E. Barillier
  • , D. Bauer
  • , K. Beattie
  • , T. Benson
  • , A. Bhatti
  • A. Biekert, T. P. Biesiadzinski, H. J. Birch, E. Bishop, G. M. Blockinger, B. Boxer, C. A.J. Brew, P. Brás, S. Burdin, M. Buuck, M. C. Carmona-Benitez, M. Carter, A. Chawla, H. Chen, J. J. Cherwinka, Y. T. Chin, N. I. Chott, M. V. Converse, R. Coronel, A. Cottle, G. Cox, D. Curran, C. E. Dahl, I. Darlington, S. Dave, A. David, J. Delgaudio, S. Dey, L. De Viveiros, L. Di Felice, C. Ding, J. E.Y. Dobson, E. Druszkiewicz, S. Dubey, S. R. Eriksen, A. Fan, S. Fayer, N. M. Fearon, N. Fieldhouse, S. Fiorucci, H. Flaecher, E. D. Fraser, T. M.A. Fruth, R. J. Gaitskell, A. Geffre, J. Genovesi, C. Ghag, A. Ghosh, R. Gibbons, S. Gokhale, J. Green, M. G.D. Van der Grinten, J. J. Haiston, C. R. Hall, T. J. Hall, S. Han, E. Hartigan-O’Connor, S. J. Haselschwardt, M. A. Hernandez, S. A. Hertel, G. Heuermann, G. J. Homenides, M. Horn, D. Q. Huang, D. Hunt, E. Jacquet, R. S. James, J. Johnson, A. C. Kaboth, A. C. Kamaha, M. Kannichankandy, D. Khaitan, A. Khazov, I. Khurana, J. Kim, Y. D. Kim, J. Kingston, R. Kirk, D. Kodroff, L. Korley, E. V. Korolkova, H. Kraus, S. Kravitz, L. Kreczko, V. A. Kudryavtsev, C. Lawes, D. S. Leonard, K. T. Lesko, C. Levy, J. Lin, A. Lindote, W. H. Lippincott, M. I. Lopes, W. Lorenzon, C. Lu, S. Luitz, P. A. Majewski, A. Manalaysay, R. L. Mannino, C. Maupin, M. E. McCarthy, G. McDowell, D. N. McKinsey, J. McLaughlin, J. B. McLaughlin, R. McMonigle, E. Mizrachi, A. Monte, M. E. Monzani, J. D.Morales Mendoza, E. Morrison, B. J. Mount, M. Murdy, A. St J. Murphy, A. Naylor, H. N. Nelson, F. Neves, A. Nguyen, C. L. O’Brien, I. Olcina, K. C. Oliver-Mallory, J. Orpwood, K. Y. Oyulmaz, K. J. Palladino, J. Palmer, N. J. Pannifer, N. Parveen, S. J. Patton, B. Penning, G. Pereira, E. Perry, T. Pershing, A. Piepke, Y. Qie, J. Reichenbacher, C. A. Rhyne, A. Richards, Q. Riffard, G. R.C. Rischbieter, E. Ritchey, H. S. Riyat, R. Rosero, T. Rushton, D. Rynders, D. Santone, A. B.M.R. Sazzad, R. W. Schnee, G. Sehr, B. Shafer, S. Shaw, T. Shutt, J. J. Silk, C. Silva, G. Sinev, J. Siniscalco, R. Smith, V. N. Solovov, P. Sorensen, J. Soria, I. Stancu, A. Stevens, K. Stifter, B. Suerfu, T. J. Sumner, M. Szydagis, D. R. Tiedt, M. Timalsina, Z. Tong, D. R. Tovey, J. Tranter, M. Trask, M. Tripathi, A. Usón, A. Vacheret, A. C. Vaitkus, O. Valentino, V. Velan, A. Wang, J. J. Wang, Y. Wang, J. R. Watson, L. Weeldreyer, T. J. Whitis, K. Wild, M. Williams, W. J. Wisniewski, L. Wolf, F. L.H. Wolfs, S. Woodford, D. Woodward, C. J. Wright, Q. Xia, J. Xu, Y. Xu, M. Yeh, D. Yeum, W. Zha, H. Zhang, E. A. Zweig
  • SLAC National Accelerator Laboratory
  • Kavli Institute for Particle Astrophysics and Cosmology
  • University College London
  • University of California
  • Imperial College London
  • University of Maryland, College Park
  • King's College London
  • STFC Rutherford Appleton Laboratory (RAL)
  • Brown University
  • University of Michigan, Ann Arbor
  • University of Zurich
  • Lawrence Berkeley National Laboratory
  • University of Wisconsin-Madison
  • University of Edinburgh
  • SUNY Albany
  • University of Coimbra
  • University of Liverpool
  • Pennsylvania State University
  • Royal Holloway University of London
  • South Dakota School of Mines & Technology
  • University of Rochester
  • South Dakota Science and Technology Authority
  • Northwestern University
  • Fermi National Accelerator Laboratory
  • University of Oxford
  • University of Bristol
  • The University of Sydney
  • Brookhaven National Laboratory
  • University of Massachusetts
  • University of Alabama
  • University of California at Los Angeles
  • Institute for Basic Science
  • University of Sheffield
  • University of Texas at Austin
  • Lawrence Livermore National Laboratory
  • Vatican Observatory
  • Black Hills State University

Research output: Contribution to journalArticlepeer-review

2 Scopus citations

Abstract

We report on a search for millicharged particles (mCPs) produced in cosmic ray atmospheric interactions using data collected during the first science run of the LUX-ZEPLIN experiment. The mCPs produced by two processes—meson decay and proton bremsstrahlung—are considered in this study. This search utilized a novel signature unique to liquid xenon (LXe) time projection chambers, allowing sensitivity to mCPs with masses ranging from 10 to 1000MeV/c2 and fractional charges between 0.001 and 0.02 of the electron charge (e). With an exposure of 60 live days and a 5.5 metric ton fiducial mass, we observed no significant excess over background. This represents the first experimental search for atmospheric mCPs and the first search for mCPs using an underground LXe experiment.

Original languageEnglish
Article number241802
JournalPhysical Review Letters
Volume134
Issue number24
DOIs
StatePublished - Jun 20 2025

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