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Search for dark matter particle interactions in an extended nuclear recoil energy window with the LUX-ZEPLIN (LZ) experiment

D.S. Akerib, A.K. Al Musalhi, B.J. Almquist, C.S. Amarasinghe, A. Ames, T. Anderson, N. Angelides, H.M. Araújo
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J.E. Armstrong, M. Arthurs, A. Baker, S. Balashov, J. Bang, J.W. Bargemann, E.E. Barillier, D. Bauer, K. Beattie, A. Beauchene, T.L. Benson, A. Bhatti, T.P. Biesiadzinski, H.J. Birch, E. Bishop, G.M. Blockinger, B. Boxer, C.A.J. Brew, P. Brás, S. Burdin, M.C. Carmona-Benitez, M. Carter, A. Chawla, J.J. Cherwinka, Y.T. Chin, S. Contreras, M.V. Converse, R. Coronel, A. Cottle, C. Coulson, G. Cox, C.E. Dahl, I. Darlington, S. Dave, J. Delgaudio, S. Desai, S. Dey, L. de Viveiros, L. Di Felice, C. Ding, J.E.Y. Dobson, E. Druszkiewicz, S. Dubey, C.L. Dunbar, S.R. Eriksen, S. Fayer, N. Fieldhouse, S. Fiorucci, H. Flaecher, E.D. Fraser, T.M.A. Fruth, P.W. Gaemers, R.J. Gaitskell, A. Geffre, J. Genovesi, C. Ghag, J. Ghamsari, A. Ghosh, S. Ghosh, R. Gibbons, S. Gokhale, J. Green, M.G.D.van der Grinten, J.J. Haiston, C.R. Hall, T. Hall, R.N. Hampp, S.J. Haselschwardt, M.A. Hernandez, S.A. Hertel, G.J. Homenides, M. Horn, T. Horoho, D.Q. Huang, W. Hulse, D. Hunt, E. Jacquet, R.S. James, K.R. Jenkins, A.C. Kaboth, A.C. Kamaha, D. Khaitan, A. Khazov, J. Kim, Y.D. Kim, D. Kodroff, Q.C. Kong, E.V. Korolkova, H. Kraus, S. Kravitz, L. Kreczko, V.A. Kudryavtsev, C. Lawes, E.B. Leon, D.S. Leonard, K.T. Lesko, C. Levy, Z. Li, J. Lin, A. Lindote, W.H. Lippincott, J. Long, M.I. Lopes, W. Lorenzon, C. Lu, S. Luitz, W. Ma, V. Mahajan, P.A. Majewski, A. Manalaysay, R.L. Mannino, R.J. Matheson, C. Maupin, M.E. McCarthy, D.N. McKinsey, J. McLaughlin, J.B. McLaughlin, B. Mitra, E. Mizrachi, M.E. Monzani, K. Morå, E. Morrison, B.J. Mount, J. Munski, M. Murdy, A.St.J. Murphy, H.N. Nelson, F. Neves, A. Nguyen, C.L. O'Brien, F.H. O'Shea, I. Olcina, K.C. Oliver-Mallory, J. Orpwood, K.Y Oyulmaz, K.J. Palladino, N.J. Pannifer, S.J. Patton, B. Penning, G. Pereira, R. Peres, E. Perry, T. Pershing, A. Piepke, S.S. Poudel, Y. Qie, J. Reichenbacher, G.R.C. Rischbieter, E. Ritchey, H.S. Riyat, R. Rosero, N.J. Rowe, T. Rushton, D. Rynders, S. Saltão, I. Sargeant, A.B.M.R. Sazzad, R.W. Schnee, G. Sehr, M. Severson B. Shafer, S. Shaw, L. Sherman, K. Shi, T. Shutt, C. Silva, G. Sinev, J. Siniscalco, A.M. Softley-Brown, V.N. Solovov, P. Sorensen, J. Soria, T.J. Sumner, M. Szydagis, C.F. Tang, K. Thieme, D.R. Tiedt, D.R. Tovey, J. Tranter, M. Trask, K. Trengove, B. Twigg, A. Usón, A.C. Vaitkus, O. Valentino, A. Wang, J.J. Wang, Y. Wang, L. Weeldreyer, T.J. Whitis, K. Wild, M. Williams, J. Winnicki, M.S. Witherell, L. Wolf, F.L.H. Wolfs, S. Woodford, D. Woodward, C.J. Wright, Q. Xia, J. Xu, Y. Xu, M. Yeh, D. Yeum, J. Young, H.D. Zenger, W. Zha, H. Zhang, T. Zhang, Y. Zhou

High Energy Physics - Experiment · Submitted 2 Sep 2026 · 73 references

Pith's verdict: An honest, hint-tier search: one 248 keV NR-candidate event at 2.6 sigma global plus world-leading NREFT limits, with the failed salting and non-blind high-energy extension as the main things a referee should probe.

T0 · AI review

How this review was made: An AI referee (deepseek/deepseek-v4-flash) read the paper on September 8, 2026 and answered a fixed list of questions about it. T0 is the starting level every paper gets. The levels describe how deeply Pith has checked the paper, never the authors.

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arXiv ID2609.02823 (version 1)
Pith IDVCO6YUAL, Pith's permanent record of this paper and its review
CitationA. Ames, A. Baker, A. Beauchene, A. Bhatti, A.B.M.R. Sazzad, A. Chawla, A.C. Kaboth, A.C. Kamaha, A. Cottle, A.C. Vaitkus, A. Geffre, A. Ghosh, A.K. Al Musalhi, A. Khazov, A. Lindote, A. Manalaysay, A.M. Softley-Brown, A. Nguyen, A. Piepke, A.St.J. Murphy, A. Us\'{o}n, A. Wang, B. Boxer, B.J. Almquist, B.J. Mount, B. Mitra, B. Penning, B. Twigg, C.A.J. Brew, C. Coulson, C. Ding, C.E. Dahl, C.F. Tang, C. Ghag, C.J. Wright, C. Lawes, C.L. Dunbar, C. Levy, C.L. O'Brien, C. Lu, C. Maupin, C.R. Hall, C.S. Amarasinghe, C. Silva, D. Bauer, D. Hunt, D. Khaitan, D. Kodroff, D.N. McKinsey, D.Q. Huang, D.R. Tiedt, D.R. Tovey, D. Rynders, D.S. Akerib, D.S. Leonard, D. Woodward, D. Yeum, E. Bishop, E.B. Leon, E.D. Fraser, E. Druszkiewicz, E.E. Barillier, E. Jacquet, E. Mizrachi, E. Morrison, E. Perry, E. Ritchey, E.V. Korolkova, F.H. O'Shea, F.L.H. Wolfs, F. Neves, G. Cox, G.J. Homenides, G.M. Blockinger, G. Pereira, G.R.C. Rischbieter, G. Sehr, G. Sinev, H.D. Zenger, H. Flaecher, H.J. Birch, H. Kraus, H.M. Ara\'{u}jo, H.N. Nelson, H.S. Riyat, H. Zhang, I. Darlington, I. Olcina, I. Sargeant, J. Bang, J.B. McLaughlin, J. Delgaudio, J.E. Armstrong, J.E.Y. Dobson, J. Genovesi, J. Ghamsari, J. Green, J.J. Cherwinka, J.J. Haiston, J.J. Wang, J. Kim, J. Lin, J. Long, J. Mclaughlin, J. Munski, J. Orpwood, J. Reichenbacher, J. Siniscalco, J. Soria, J. Tranter, J.W. Bargemann, J. Winnicki, J. Xu, J. Young, K. Beattie, K.C. Oliver-Mallory, K.J. Palladino, K. Mor\r{a}, K.R. Jenkins, K. Shi, K. Thieme, K.T. Lesko, K. Trengove, K. Wild, K.Y Oyulmaz, L. de Viveiros, L. Di Felice, L. Kreczko, L. Sherman, L. Weeldreyer, L. Wolf, M.A. Hernandez, M. Arthurs, M. Carter, M.C. Carmona-Benitez, M.E. McCarthy, M.E. Monzani, M.G.D.van der Grinten, M. Horn, M.I. Lopes, M. Murdy, M. Severson B. Shafer, M.S. Witherell, M. Szydagis, M. Trask, M.V. Converse, M. Williams, M. Yeh, N. Angelides, N. Fieldhouse, N.J. Pannifer, N.J. Rowe, O. Valentino, P.A. Majewski, P. Br\'{a}s, P. Sorensen, P.W. Gaemers, Q.C. Kong, Q. Xia, R. Coronel, R. Gibbons, R.J. Gaitskell, R.J. Matheson, R.L. Mannino, R.N. Hampp, R. Peres, R. Rosero, R.S. James, R.W. Schnee, S.A. Hertel, S. Balashov, S. Burdin, S. Contreras, S. Dave, S. Desai, S. Dey, S. Dubey, S. Fayer, S. Fiorucci, S. Ghosh, S. Gokhale, S.J. Haselschwardt, S.J. Patton, S. Kravitz, S. Luitz, S.R. Eriksen, S. Salt\~{a}o, S. Shaw, S.S. Poudel, S. Woodford, T. Anderson, T. Hall, T. Horoho, T.J. Sumner, T.J. Whitis, T.L. Benson, T.M.A. Fruth, T.P. Biesiadzinski, T. Pershing, T. Rushton, T. Shutt, T. Zhang, V.A. Kudryavtsev, V. Mahajan, V.N. Solovov, W.H. Lippincott, W. Hulse, W. Lorenzon, W. Ma, W. Zha, Y.D. Kim, Y. Qie, Y.T. Chin, Y. Wang, Y. Xu, Y. Zhou, Z. Li. "Search for dark matter particle interactions in an extended nuclear recoil energy window with the LUX-ZEPLIN (LZ) experiment." arXiv:2609.02823 (2026). https://pith.science/paper/VCO6YUAL
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Referee report
The paper

The paper claims

LUX-ZEPLIN observes a high-energy nuclear recoil event that deviates from background expectations at 2.6σ global significance.

The reading

The paper reports a search for dark matter interactions in an extended nuclear recoil energy window up to 270 keV with 2.84 tonne-years of LUX-ZEPLIN data. One event consistent with a 248 keV nuclear recoil is observed in a region where the known background expectation is very low. A profile likelihood ratio test finds tension with the background-only hypothesis at a local significance of 3.4σ, reducing to 2.6σ after accounting for the look-elsewhere effect. The event can be described by several effective field theory or inelastic dark matter models, but a definitive conclusion requires more data. If the event is due to dark matter, it would imply interactions with non-standard momentum dependence or an inelastic scattering channel.

What carries the argument

The analysis extends the nuclear recoil energy window to approximately 270 keV, enabling sensitivity to momentum-dependent and inelastic dark matter interactions that have larger high-energy recoil fractions than standard spin-independent models. The detector response is modeled using a tuned version of NEST v2.4.5, and the background includes a dedicated multiple-scintillation single-ionization (MSSI) component validated with sideband data. An unbinned extended maximum likelihood fit to three event samples (science, prompt veto, delayed veto) uses a profile likelihood ratio test with nuisance parameters to assess signal hypotheses.

Extended reading notes

Core claim

With an exposure of 2.84 tonne-years, the LZ experiment observes one event in the science sample that lies in the nuclear recoil band with S1c = 540.1 phd and S2c = 9268 phd, corresponding to an elastic nuclear recoil energy of 248 ± 23 (stat) ± 23 (sys) keV. The event is 6.7σ below the ER band median and 1.5σ below the NR band median at that S1c. The background model predicts 0.0106 ± 0.0008 (sys) events in the relevant projection bin, making this a low-probability fluctuation under the background-only hypothesis. The incorporated look-elsewhere effect across 293 distinct signal models yields a global significance of 2.6σ, with maximum local significance of 3.4σ typically seen for WIMP masses above 200 GeV/c². The collaboration provides 90% confidence level intervals on coupling strengths for 20 Lagrangian operators and two inelastic operators, setting world-leading limits on all tested models.

Load-bearing premise

The geometry and volume of the charge-dead regions near the TPC walls, which produce multiple-scintillation single-ionization (MSSI) background, are modeled with a 100% uncertainty covering up to 0.6% of the active volume; if the actual charge-dead region is larger or the modeling is incorrect, the MSSI background could be significantly higher, potentially explaining the observed event.

Editorial extensions

If this is right

  • If the event is confirmed with additional exposure, it would provide evidence for dark matter with a non-standard recoil spectrum, such as that predicted by certain NREFT operators or inelastic models.
  • The resulting upper limits are the strongest to date for dozens of effective field theory and inelastic dark matter interactions in the explored mass range.
  • The analysis demonstrates the feasibility of probing high-energy nuclear recoils in liquid xenon, motivating similar searches in other direct-detection experiments.
  • A larger dataset or a second similar event would allow a more robust test of the background model, especially the MSSI component, which carries a factor-of-two uncertainty.
  • The event may constrain theoretical models, such as Higgsino-like or magnetic-moment interactions, providing a target for future collider and astroparticle searches.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • The 2.6σ global significance is below the conventional 3σ evidence threshold, so chance coincidence with a rare background remains a viable explanation; continued data-taking will be decisive.
  • If the event is real, it would likely point to a dark matter particle with mass ≳ 200 GeV/c² and an interaction that suppresses low-energy recoils (e.g., momentum-dependent or inelastic), because a standard spin-independent WIMP would produce many more events at lower energies.
  • The MSSI background, though estimated to be very low in the signal region, could be underestimated if the charge-dead volume is larger than modeled; more precise electrostatic simulations or direct measurements of the dead-layer thickness would strengthen future analyses.
  • The fact that no other high-energy NR-like events appear in the 5.4-tonne sideband or the veto samples supports the background model, but also means that a single event at high energy is statistically fragile.
Original abstract

We report on a search for dark matter particles interacting with xenon nuclei in an exposure of 2.84 tonne-years with the LUX-ZEPLIN (LZ) experiment. An extended nuclear recoil energy window up to approximately 270 keV enables searches for effective field theory and inelastic models of dark matter where high-energy recoils account for a larger fraction of the predicted recoil spectrum compared to the nominal spin independent interaction. We observe one event with characteristics consistent with a nuclear recoil of $248\pm23\,\mathrm{(stat)}\pm23\,\mathrm{(sys)}$ keV, in a region where the known background expectation is low. A profile likelihood ratio test finds tension with the background-only hypothesis at a global significance of 2.6$\sigma$ when accounting for look-elsewhere effects, with a maximum local significance of 3.4$\sigma$ across the models tested. We describe the analysis and event of interest, the background model used in the statistical inference, and detail several of the rare background topologies considered.

The compiled record

The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,496 input tokens.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.42 · human participants 0.02 · controlled comparison 0.37 · randomized assignment 0.01 · states quantitative result 0.98 · compares with prior results 0.29 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

We report on a search for dark matter particles interacting with xenon nuclei in an exposure of 2.84 tonne-years with the LUX-ZEPLIN (LZ) experiment. An extended nuclear recoil energy window up to approximately 270 keV enables searches for effective field theory and inelastic models of dark matter where high-energy recoils account for a larger fraction of the predicted recoil spectrum compared to the nominal spin independent interaction. We observe one event with characteristics consistent with a nuclear recoil of $248\pm23\,\mathrm{(stat)}\pm23\,\mathrm{(sys)}$ keV, in a region where the known background expectation is low. A profile likelihood ratio test finds tension with the background-only hypothesis at a global significance of 2.6$\sigma$ when accounting for look-elsewhere effects, with a maximum local significance of 3.4$\sigma$ across the models tested. We describe the analysis and event of interest, the background model used in the statistical inference, and detail several of the rare background topologies considered.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 We report on a search for dark matter particles interacting with xenon nuclei in an exposure of 2.84 tonne-years with the LUX-ZEPLIN (LZ) experiment. contribution 0.94 0.97 0.06 asserted 0.98
s1 An extended nuclear recoil energy window up to approximately 270 keV enables searches for effective field theory and inelastic models of dark matter where high-energy recoils account for a larger fraction of the predicted recoil spectrum compared to the nominal spin independent interaction. method 0.65 0.64 0.04 asserted 0.87
s2 We observe one event with characteristics consistent with a nuclear recoil of $248\pm23\,\mathrm{(stat)}\pm23\,\mathrm{(sys)}$ keV, in a region where the known background expectation is low. result 1.00 0.96 0.10 hedged possibility 0.64
s3 A profile likelihood ratio test finds tension with the background-only hypothesis at a global significance of 2.6$\sigma$ when accounting for look-elsewhere effects, with a maximum local significance of 3.4$\sigma$ across the models tested. result 1.00 0.96 0.32 asserted 0.97
s4 We describe the analysis and event of interest, the background model used in the statistical inference, and detail several of the rare background topologies considered. method 0.58 0.84 0.02 asserted 0.86

What kind of paper the classifier reports this is: empirical study 1.00 · evidence from observation or experiment 0.96.

What was examined, and what was not

sources read
  • arXiv listing abstract v1
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

Figures
Figure 1. FIG. 1. Nuclear recoil energy spectra for the two interactions
Figure 2. FIG. 2. Calibration events in
Figure 4. FIG. 4. Black points show the WIMP search data from the
Figure 5. FIG. 5. Comparison between the data in the
Figure 6. FIG. 6. Two-sided 90% confidence-level intervals (solid-black)

Showing 5 of the paper's 6 figures. See all figures in the PDF ↗ Figures reproduced from arXiv:2609.02823 by the authors.

References

Discussion

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