Projected sensitivity of the LUX-ZEPLIN experiment to the 0 ν β β decay of Xe 136
2020; American Physical Society; Volume: 102; Issue: 1 Linguagem: Inglês
10.1103/physrevc.102.014602
ISSN2470-0002
AutoresD. S. Akerib, C. Akerlof, A. Alqahtani, S. Alsum, Tyler Anderson, N. Angelides, H. M. Araújo, J. E. Armstrong, M. Arthurs, X. Bai, J. Balajthy, S. Balashov, J. Bang, A. Baxter, J. R. Bensinger, E. P. Bernard, A. Bernstein, A. Bhatti, A. Biekert, T. P. Biesiadzinski, H. J. Birch, K. E. Boast, B. Boxer, P. Brás, J. H. Buckley, V. V. Bugaev, S. Burdin, J.K. Busenitz, R. Cabrita, C. Carels, D. Carlsmith, M. C. Carmona-Benitez, M. Cascella, C. Chan, N. Chott, A. Cole, A. Cottle, J. E. Cutter, C. E. Dahl, L. de Viveiros, J. E. Y. Dobson, E. Druszkiewicz, T. K. Edberg, S. R. Eriksen, A. Fan, S. Fiorucci, H. Flaecher, E. D. Fraser, T. Fruth, R. J. Gaitskell, J. Genovesi, C. Ghag, E. F. Gibson, M. G. D. Gilchriese, S. Gokhale, M. G. D. van der Grinten, C. Hall, Aaron W. Harrison, S. J. Haselschwardt, S. A. Hertel, J. Y-K. Hor, M. Horn, D. Q. Huang, C. M. Ignarra, O. Jahangir, W. Ji, J. Johnson, A. C. Kaboth, A. Kamaha, K. Kamdin, K. Kazkaz, D. Khaitan, A. Khazov, I. Khurana, Charles D. Kocher, L. Korley, E. V. Korolkova, J. Kras, H. Kraus, S. Kravitz, L. Kreczko, B. Krikler, V. A. Kudryavtsev, E. Leason, J. Lee, D. S. Leonard, K. T. Lesko, C. Levy, J. Li, J. Liao, F.-T. Liao, J. Lin, A. Lindote, R. Linehan, W. H. Lippincott, R. Liu, X. Liu, C. Loniewski, I. Lopes, B. López Paredes, W. Lorenzon, S. Luitz, Justin Lyle, P. A. Majewski, A. Manalaysay, L. Manenti, R. L. Mannino, N. Marangou, M. F. Marzioni, D. N. McKinsey, J. Lin, Yue Meng, E. H. Miller, E. Mizrachi, A. Monte, M. E. Monzani, J. A. Morad, E. Morrison, B. J. Mount, A. St. J. Murphy, D. Naim, A. Naylor, C. Nedlik, C. Nehrkorn, H. Nelson, F. Neves, J. A. Nikoleyczik, A. Nilima, K. O’Sullivan, I. Olcina, K. C. Oliver-Mallory, S. K. Pal, K. J. Palladino, J. D. Palmer, N. Parveen, E. K. Pease, B. Penning, G. Pereira, K. Pushkin, J. Reichenbacher, C. Rhyne, Q. Riffard, G. R. C. Rischbieter, R. Rosero, P. Rossiter, G. Rutherford, D. Santone, A. B. M. R. Sazzad, R. W. Schnee, M. Schubnell, Danelle K. Seymour, S. Shaw, T. Shutt, J. J. Silk, C. Silva, R. Smith, M. Solmaz, V. N. Solovov, P. Sørensen, I. Stancu, A. Stevens, K. Stifter, T. J. Sumner, N. Swanson, M. Szydagis, Mustafa Özgür Tan, WC Taylor, R. Taylor, Dylan Temples, P. A. Terman, D. R. Tiedt, M. Timalsina, A. Tomás, M. Tripathi, D. R. Tronstad, W. Turner, L. Tvrznikova, U. Utku, A. Vacheret, Audrius Vaitkus, J.J. Wang, W. Wang, J. R. Watson, R. C. Webb, R. G. White, T. J. Whitis, F. L. H. Wolfs, D. Woodward, X. Xiang, Jing Xu, M. Yeh, P. Zarzhitsky,
Tópico(s)Dark Matter and Cosmic Phenomena
ResumoThe LUX-ZEPLIN (LZ) experiment will enable a neutrinoless double $\ensuremath{\beta}$ decay search in parallel to the main science goal of discovering dark matter particle interactions. We report the expected LZ sensitivity to $^{136}\mathrm{Xe}$ neutrinoless double $\ensuremath{\beta}$ decay, taking advantage of the significant ($>600$ kg) $^{136}\mathrm{Xe}$ mass contained within the active volume of LZ without isotopic enrichment. After 1000 live-days, the median exclusion sensitivity to the half-life of $^{136}\mathrm{Xe}$ is projected to be $1.06\ifmmode\times\else\texttimes\fi{}{10}^{26}$ years (90% confidence level), similar to existing constraints. We also report the expected sensitivity of a possible subsequent dedicated exposure using 90% enrichment with $^{136}\mathrm{Xe}$ at $1.06\ifmmode\times\else\texttimes\fi{}{10}^{27}$ years.
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