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. 2025 Jun 20;134(24):241801.
doi: 10.1103/nr92-jvt3.

New Constraints on Cosmic Ray-Boosted Dark Matter from the LUX-ZEPLIN Experiment

J Aalbers  1   2 D S Akerib  1   2 A K Al Musalhi  3 F Alder  3 C S Amarasinghe  4 A Ames  1   2 T J Anderson  1   2 N Angelides  5 H M Araújo  5 J E Armstrong  6 M Arthurs  1   2 A Baker  5   7 S Balashov  8 J Bang  9 J W Bargemann  4 E E Barillier  10   11 K Beattie  12 T Benson  13 A Bhatti  6 A Biekert  12   14 T P Biesiadzinski  1   2 H J Birch  10   11 E Bishop  15 G M Blockinger  16 B Boxer  17 C A J Brew  8 P Brás  18 S Burdin  19 M Buuck  1   2 M C Carmona-Benitez  20 M Carter  19 A Chawla  21 H Chen  12 J J Cherwinka  13 Y T Chin  20 N I Chott  22 M V Converse  23 R Coronel  1   2 A Cottle  3 G Cox  24 D Curran  24 C E Dahl  25   26 I Darlington  3 S Dave  3 A David  3 J Delgaudio  24 S Dey  27 L de Viveiros  20 L Di Felice  5 C Ding  9 J E Y Dobson  3   7 E Druszkiewicz  23 S Dubey  9 S R Eriksen  28 A Fan  1   2 N M Fearon  27 N Fieldhouse  27 S Fiorucci  12 H Flaecher  28 E D Fraser  19 T M A Fruth  29 R J Gaitskell  9 A Geffre  24 J Genovesi  20 C Ghag  3 R Gibbons  12   14 S Gokhale  30 J Green  27 M G D van der Grinten  8 J J Haiston  22 C R Hall  6 T Hall  19 S Han  1   2 E Hartigan-O'Connor  9 S J Haselschwardt  10 M A Hernandez  10   11 S A Hertel  31 G Heuermann  10 G J Homenides  32 M Horn  24 D Q Huang  33 D Hunt  27 E Jacquet  5 R S James  3 M K Kannichankandy  16 A C Kaboth  21 A C Kamaha  33 D Khaitan  23 A Khazov  8 J Kim  4 Y D Kim  34 J Kingston  17 R Kirk  9 D Kodroff  12 L Korley  10 E V Korolkova  35 H Kraus  27 S Kravitz  36 L Kreczko  28 V A Kudryavtsev  35 C Lawes  7 D S Leonard  34 K T Lesko  12 C Levy  16 J Lin  12   14 A Lindote  18 W H Lippincott  4 M I Lopes  18 W Lorenzon  10 C Lu  9 S Luitz  1   2 P A Majewski  8 A Manalaysay  12 R L Mannino  37 C Maupin  24 M E McCarthy  23 G McDowell  10 D N McKinsey  12   14 J McLaughlin  25 J B McLaughlin  3 R McMonigle  16 E Mizrachi  6   37 M E Monzani  1   2   38 E Morrison  22 B J Mount  39 M Murdy  31 A St J Murphy  15 H N Nelson  4 F Neves  18 A Nguyen  15 C L O'Brien  36 I Olcina  12   14 K C Oliver-Mallory  5 J Orpwood  35 K Y Oyulmaz  15 K J Palladino  27 J Palmer  21 N J Pannifer  28 N Parveen  16 S J Patton  12 B Penning  10   11 G Pereira  18 E Perry  12 T Pershing  37 A Piepke  32 Y Qie  23 J Reichenbacher  22 C A Rhyne  9 G R C Rischbieter  10   11 E Ritchey  6 H S Riyat  15 R Rosero  30 T Rushton  35 D Rynders  24 D Santone  21   27 A B M R Sazzad  32 R W Schnee  22 G Sehr  36 B Shafer  6 S Shaw  15 K Shi  10 T Shutt  1   2 J J Silk  6 C Silva  18 J Siniscalco  3 R Smith  12   14 V N Solovov  18 P Sorensen  12 J Soria  12   14 I Stancu  32 A Stevens  3   5 K Stifter  26 B Suerfu  12   14 T J Sumner  5 A Swain  27 M Szydagis  16 D R Tiedt  24 M Timalsina  12 Z Tong  5 D R Tovey  35 J Tranter  35 M Trask  4 M Tripathi  17 A Usón  15 A C Vaitkus  9 O Valentino  5 V Velan  12 A Wang  1   2 J J Wang  32 Y Wang  12   14 J R Watson  12   14 L Weeldreyer  32 T J Whitis  4 K Wild  20 M Williams  10 W J Wisniewski  1 L Wolf  21 F L H Wolfs  23 S Woodford  19 D Woodward  12   20 C J Wright  28 Q Xia  12 J Xu  37 Y Xu  33 M Yeh  30 D Yeum  6 W Zha  20 H Zhang  15 LZ Collaboration
Affiliations

New Constraints on Cosmic Ray-Boosted Dark Matter from the LUX-ZEPLIN Experiment

J Aalbers et al. Phys Rev Lett. .

Abstract

While dual-phase xenon time projection chambers have driven the sensitivity toward weakly interacting massive particles at the GeV/c^{2} to TeV/c^{2} mass scale, the scope for sub-GeV/c^{2} dark matter particles is hindered by a limited nuclear recoil energy detection threshold. One approach to probe for lighter candidates is to consider cases where they have been boosted by collisions with cosmic rays in the Milky Way, such that the additional kinetic energy lifts their induced signatures above the nominal threshold. In this Letter, we report first results of a search for cosmic ray-boosted dark matter (CRDM) with a combined 4.2 metric ton/yr exposure from the LUX-ZEPLIN experiment. We observe no excess above the expected backgrounds and establish world-leading constraints on the spin-independent CRDM-nucleon cross section as small as 3.9×10^{-33} cm^{2} at 90% confidence level for sub-GeV/c^{2} masses.

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