Two-neutrino double electron capture of <sup>124</sup>Xe in the first LUX-ZEPLIN exposure

Abstract The broad physics reach of the LUX-ZEPLIN (LZ) experiment covers rare phenomena beyond the direct detection of dark matter. We report precise measurements of the extremely rare decay of 124 Xe through the process of two-neutrino double electron capture, utilizing a 1.39 kg × yr isotopic exposure from the first LZ science run. A half-life of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msubsup> <mml:mi>T</mml:mi> <mml:mrow> <mml:mn>1</mml:mn> <mml:mo>/</mml:mo> <mml:mn>2</mml:mn> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> <mml:mi>ν</mml:mi> <mml:mn>2</mml:mn> <mml:mi>EC</mml:mi> </mml:mrow> </mml:msubsup> <mml:mspace width="0.25em"/> <mml:mo>=</mml:mo> <mml:mo stretchy="false">(</mml:mo> <mml:mn>1.09</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.1</mml:mn> <mml:msub> <mml:mn>4</mml:mn> <mml:mrow> <mml:mspace width="0.1em"/> <mml:mtext>stat</mml:mtext> </mml:mrow> </mml:msub> <mml:mo>±</mml:mo> <mml:mn>0.0</mml:mn> <mml:msub> <mml:mn>5</mml:mn> <mml:mrow> <mml:mtext>sys</mml:mtext> <mml:mspace width="0.1em"/> </mml:mrow> </mml:msub> <mml:mo stretchy="false">)</mml:mo> <mml:mo>×</mml:mo> <mml:mn>1</mml:mn> <mml:msup> <mml:mn>0</mml:mn> <mml:mn>22</mml:mn> </mml:msup> <mml:mspace width="0.25em"/> <mml:mi>yr</mml:mi> </mml:math> is observed with a statistical significance of 8.3 σ , in agreement with literature. First empirical measurements of the KK capture fraction relative to other K-shell modes were conducted, and demonstrate consistency with respect to recent signal models at the 1.4 σ level.

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Journal
Journal of Physics G Nuclear and Particle Physics
Published
2024-12-06
DOI
https://doi.org/10.1088/1361-6471/ad9039
Citations
6
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
3.96

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article

Two-neutrino double electron capture of 124Xe in the first LUX-ZEPLIN exposure

J. W. Bargemann, M. Yeh, K. J. Palladino, R. L. Kirk et al.
6 citations
Journal of Physics G Nuclear and Particle Physics
Dark Matter and Cosmic Phenomena
3.96
article

Two-neutrino double electron capture of 124Xe in the first LUX-ZEPLIN exposure

J. W. Bargemann, M. Yeh, K. J. Palladino, R. L. Kirk, A. Biekert, D. Q. Huang, E. Hartigan-O’Connor, A. K. Al Musalhi, Tyler Anderson, W. Zha, L. Kreczko, J. Lin, R. Gibbons, F. Alder, H. J. Birch, Donald F. Hunt, S. Shaw, V. N. Solovov, E. D. Fraser, G. Pereira, N. Parveen, D. S. Akerib, R. L. Mannino, D. R. Tovey, Jing Xu, D. Yeum, M. Arthurs, T. Pershing, E. Mizrachi, Audrius Vaitkus, V. Velan, T. P. Biesiadzinski, E. Morrison, B. J. Mount, D. Khaitan, E. Jacquet, P. Sørensen, S. Kravitz, L. Korley, V. A. Kudryavtsev, N. Fieldhouse, S. A. Hertel, J. B. Mclaughlin, John M. DelGaudio, M.A. Hernández, D. Kodroff, D. Santone, A. Chawla, M. Murdy, C. Hall, S. Balashov, S. Woodford, M. Szydagis, Graham McDowell, Jemima Tranter, Erin Bishop, W. J. Wisniewski, E. A. Zweig, J. Genovesi, J. E. Y. Dobson, E. Druszkiewicz, J. J. Haiston, F. L. H. Wolfs, B. Suerfu, A. Cottle, B. Boxer, A S J Murphy, C. A. Rhyne, M. C. Carmona-Benitez, M. Trask, R. W. Schnee, I. Olcina, Ruben Coronel, K. Wild, L. de Viveiros, R. S. James, Alexander A. Baker, I. Lopes, M. Williams, D. Rynders, Simon Patton, Levi John Wolf, Q. Xia, D. N. McKinsey, Chris J. Wright, Jaebak Kim, K. T. Lesko, J J Wang, J. Aalbers, H. S. Riyat, F. Neves, Edwin L. Ritchey, Q. Riffard, A. Kamaha, C. Silva, G. R. C. Rischbieter, C E Dahl, G. M. Blockinger, M. V. Converse, K. Beattie, B. Penning, T. Fruth, D. Woodward, C. S. Amarasinghe, A. B. M. R. Sazzad, T. Rushton, H. M. Araújo, H. Nelson, N. M. Fearon, A. Geffre, M. E. Monzani, K. C. Oliver-Mallory, P. Brás, S. J. Haselschwardt, A. Manalaysay, A. Lindote, C. Maupin, M. Horn, S. Burdin, S. Dubey, S. Fiorucci, S. R. Eriksen, M. Buuck, C. Ghag, T. J. Sumner, Jennifer Kingston, W. Lorenzon, W. H. Lippincott, A. Ames, L. Weeldreyer, N. J. Pannifer, G. J. Homenides, R. McMonigle, E. E. Barillier, J. Siniscalco, O. Valentino, L. Di Felice, M. Kannichankandy, Andrew Wang, Ding Chen, Michael Carter, Jonathan Green, Young Dong Kim, A. Bhatti, J. P. Johnson, D. S. Leonard, J. Soria, Jean Watson, Sourav Dey, M. McCarthy, S. Luitz, N. Chott, A. Nguyen, K. Y. Oyulmaz, G. Sehr, C. L. O'Brien, A. Naylor, I. Khurana, J. D. Palmer, H. Kraus, E. V. Korolkova, A. Monte, C. Lu, S. Han, K. Stifter, A. C. Kaboth, A. David, J. J. Silk, J. Orpwood, A. Vacheret, R. J. E. Smith, A. Stevens, T. Shutt, J. E. Armstrong, C. Levy, R. J. Gaitskell, C. Brew, Z Tong, P. A. Majewski, A. Piepke, J. Reichenbacher, G. Heuermann, D. R. Tiedt, H. Flaecher, M. Timalsina, M. Tripathi, G. Sinev, G. A. Cox, M. G. D. van der Grinten, Y. T. Chin, A. Khazov, T. J. Whitis, S. Gokhale, N. Angelides, J. Bang, D. Curran, B.D. Shafer, A. Fan, E Perry, Y. Qie, R. Rosero, H Chen, Y. Xu, Y. Wang
article en
6 citations

Abstract

Abstract The broad physics reach of the LUX-ZEPLIN (LZ) experiment covers rare phenomena beyond the direct detection of dark matter. We report precise measurements of the extremely rare decay of 124 Xe through the process of two-neutrino double electron capture, utilizing a 1.39 kg × yr isotopic exposure from the first LZ science run. A half-life of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msubsup> <mml:mi>T</mml:mi> <mml:mrow> <mml:mn>1</mml:mn> <mml:mo>/</mml:mo> <mml:mn>2</mml:mn> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> <mml:mi>ν</mml:mi> <mml:mn>2</mml:mn> <mml:mi>EC</mml:mi> </mml:mrow> </mml:msubsup> <mml:mspace width="0.25em"/> <mml:mo>=</mml:mo> <mml:mo stretchy="false">(</mml:mo> <mml:mn>1.09</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.1</mml:mn> <mml:msub> <mml:mn>4</mml:mn> <mml:mrow> <mml:mspace width="0.1em"/> <mml:mtext>stat</mml:mtext> </mml:mrow> </mml:msub> <mml:mo>±</mml:mo> <mml:mn>0.0</mml:mn> <mml:msub> <mml:mn>5</mml:mn> <mml:mrow> <mml:mtext>sys</mml:mtext> <mml:mspace width="0.1em"/> </mml:mrow> </mml:msub> <mml:mo stretchy="false">)</mml:mo> <mml:mo>×</mml:mo> <mml:mn>1</mml:mn> <mml:msup> <mml:mn>0</mml:mn> <mml:mn>22</mml:mn> </mml:msup> <mml:mspace width="0.25em"/> <mml:mi>yr</mml:mi> </mml:math> is observed with a statistical significance of 8.3 σ , in agreement with literature. First empirical measurements of the KK capture fraction relative to other K-shell modes were conducted, and demonstrate consistency with respect to recent signal models at the 1.4 σ level.

Journal of Physics G Nuclear and Particle PhysicsVol. 52(1)
Northwestern University (US), Lawrence Livermore National Laboratory (US), Rutherford Appleton Laboratory (GB), The University of Sydney (AU), Pennsylvania State University (US), Fermi National Accelerator Laboratory (US), University of Liverpool (GB), Lawrence Berkeley National Laboratory (US), University of California, Santa Barbara (US), University of California, Los Angeles (US), University of Alabama (US), Royal Holloway University of London (GB), South Dakota School of Mines and Technology (US), Brookhaven National Laboratory (US), University of Zurich (CH), University of Massachusetts Amherst (US), Brown University (US), University of Michigan (US), LIP - Laboratory of Instrumentation and Experimental Particle Physics (PT), SLAC National Accelerator Laboratory (US), University of Bristol (GB), University at Albany, State University of New York (US), University of Oxford (GB), Kavli Institute for Particle Astrophysics and Cosmology (US), Lawrence Livermore National Security (US), Vatican Observatory (IT), South Dakota Science and Technology Authority (US), University College London (GB), Imperial College London (GB), University of Rochester (US), University of Maryland, College Park (US), Black Hills State University (US), University of Coimbra (PT), University of California, Davis (US), The University of Texas at Austin (US), University of Sheffield (GB), University of California, Berkeley (US), University of Edinburgh (GB)
National Science Foundation, U.S. Department of Energy, UK Research and Innovation, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Institute for Basic Science, Office of Science, Science and Technology Facilities Council, Fundação para a Ciência e a Tecnologia, High Energy Physics
Openalex Percentile: Top 5%
Dark Matter and Cosmic Phenomena
3.96
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