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1. Light dark matter constraints from SuperCDMS HVeV detectors operated underground with an anticoincidence event selection

   https://doi.org/10.1103/PhysRevD.111.012006  

   Albakry, M F; Alkhatib, I; Alonso-González, D; Amaral, D_W P; Anczarski, J; Aralis, T; Aramaki, T; Arnquist, I J; Ataee_Langroudy, I; Azadbakht, E; et al (January 2025, Physical Review D)

   This article presents constraints on dark-matter-electron interactions obtained from the first underground data-taking campaign with multiple SuperCDMS HVeV detectors operated in the same housing. An exposure of $7.63\mathrm{g}\text{−}\mathrm{days}$ is used to set upper limits on the dark-matter-electron scattering cross section for dark matter masses between 0.5 and $1000\mathrm{MeV}/c^2$ , as well as upper limits on dark photon kinetic mixing and axionlike particle axioelectric coupling for masses between 1.2 and $23.3\mathrm{eV}/c^2$ . Compared to an earlier HVeV search, sensitivity was improved as a result of an increased overburden of 225 meters of water equivalent, an anticoincidence event selection, and better pile-up rejection. In the case of dark-matter-electron scattering via a heavy mediator, an improvement by up to a factor of 25 in cross section sensitivity was achieved. Published by the American Physical Society2025 

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2. First Search for Ultralight Dark Matter Using a Magnetically Levitated Particle

   https://doi.org/10.1103/PhysRevLett.134.251001  

   Amaral, Dorian_W P; Uitenbroek, Dennis G; Oosterkamp, Tjerk H; Tunnell, Christopher D (June 2025, Physical Review Letters)

   We perform the first search for ultralight dark matter using a magnetically levitated particle. A submillimeter permanent magnet is levitated in a superconducting trap with a measured force sensitivity of $0.2\mathrm{fN}/\sqrt{\mathrm{Hz}}$ . We find no evidence of a signal and derive limits on dark matter coupled to the difference between baryon and lepton number, $B-L$ , in the mass range $(1.10360-1.10485)\times {10}^{-13}\mathrm{eV}/c^2$ . Our most stringent limit on the coupling strength is $g_{B-L}\lesssim 2.98\times {10}^{-21}$ . We propose the POLONAISE (Probing Oscillations using Levitated Objects for Novel Accelerometry In Searches of Exotic physics) experiment, which features short-, medium-, and long-term upgrades that will give us leading sensitivity in a wide mass range, demonstrating the promise of this novel quantum sensing technology in the hunt for dark matter. Published by the American Physical Society2025 

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3. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory

   https://doi.org/10.1103/PhysRevD.109.L081101  

   Abdul_Halim, A; Abreu, P; Aglietta, M; Allekotte, I; Almeida_Cheminant, K; Almela, A; Aloisio, R; Alvarez-Muñiz, J; Ammerman_Yebra, J; Anastasi, G A; et al (April 2024, Physical Review D)

   Dark matter particles could be superheavy, provided their lifetime is much longer than the age of the Universe. Using the sensitivity of the Pierre Auger Observatory to ultrahigh energy neutrinos and photons, we constrain a specific extension of the Standard Model of particle physics that meets the lifetime requirement for a superheavy particle by coupling it to a sector of ultralight sterile neutrinos. Our results show that, for a typical dark coupling constant of 0.1, the mixing angle ${\theta }_m$ between active and sterile neutrinos must satisfy, roughly, ${\theta }_m\lesssim 1.5\times {10}^{-6}(M_X/{10}^9\mathrm{GeV}{)}^{-2}$ for a mass $M_X$ of the dark-matter particle between ${10}^8\mathrm{GeV}$ and ${10}^{11}\mathrm{GeV}$ . Published by the American Physical Society2024 

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4. First Search for Light Dark Matter in the Neutrino Fog with XENONnT

   https://doi.org/10.1103/PhysRevLett.134.111802  

   Aprile, E; Aalbers, J; Abe, K; Ahmed_Maouloud, S; Althueser, L; Andrieu, B; Angelino, E; Antón_Martin, D; Arneodo, F; Baudis, L; et al (March 2025, Physical Review Letters)

   We search for dark matter (DM) with a mass $[3,12]\mathrm{GeV}/c^2$ using an exposure of $3.51\mathrm{tonne}\hspace{0.17em}\mathrm{year}$ with the XENONnT experiment. We consider spin-independent DM-nucleon interactions mediated by a heavy or light mediator, spin-dependent DM-neutron interactions, momentum-dependent DM scattering, and mirror DM. Using a lowered energy threshold compared to the previous weakly interacting massive particle search, a blind analysis of [0.5, 5.0] keV nuclear recoil events reveals no significant signal excess over the background. XENONnT excludes spin-independent DM-nucleon cross sections $>2.5\times {10}^{-45}{\mathrm{cm}}^2$ at 90% confidence level for $6\mathrm{GeV}/c^2$ DM. In the considered mass range, the DM sensitivity approaches the “neutrino fog,” the limitation where neutrinos produce a signal that is indistinguishable from that of light DM-xenon nucleus scattering. Published by the American Physical Society2025 

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5. Effective field theory and inelastic dark matter results from XENON1T

   https://doi.org/10.1103/PhysRevD.109.112017  

   Aprile, E; Abe, K; Agostini, F; Ahmed_Maouloud, S; Althueser, L; Andrieu, B; Angelino, E; Angevaare, J R; Antochi, V C; Antón_Martin, D; et al (June 2024, Physical Review D)

   In this work, we expand on the XENON1T nuclear recoil searches to study the individual signals of dark matter interactions from operators up to dimension eight in a chiral effective field theory (ChEFT) and a model of inelastic dark matter (iDM). We analyze data from two science runs of the XENON1T detector totaling $1\mathrm{t}\times \mathrm{yr}$ exposure. For these analyses, we extended the region of interest from $[4.9,40.9]{\mathrm{keV}}_{\mathrm{NR}}$ to $[4.9,54.4]{\mathrm{keV}}_{\mathrm{NR}}$ to enhance our sensitivity for signals that peak at nonzero energies. We show that the data are consistent with the background-only hypothesis, with a small background overfluctuation observed peaking between 20 and $50{\mathrm{keV}}_{\mathrm{NR}}$ , resulting in a maximum local discovery significance of $1.7\sigma$ for the $\mathrm{Vector}\otimes {\text{Vector}}_{\text{strange}}$ ChEFT channel for a dark matter particle of $70\mathrm{GeV}/c^2$ and $1.8\sigma$ for an iDM particle of $50\mathrm{GeV}/c^2$ with a mass splitting of $100\mathrm{keV}/c^2$ . For each model, we report 90% confidence level upper limits. We also report upper limits on three benchmark models of dark matter interaction using ChEFT where we investigate the effect of isospin-breaking interactions. We observe rate-driven cancellations in regions of the isospin-breaking couplings, leading to up to 6 orders of magnitude weaker upper limits with respect to the isospin-conserving case. Published by the American Physical Society2024 

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