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Celestino-Ramirez, J. M., Escrihuela, F. J., Flores, L. J., Miranda, O. G., & Sanchez-Velez, R. (2026). Searching for generalized neutrino interactions in direct detection experiments with EνES. J. High Energy Phys., 05(5), 71–14pp.
Abstract: We investigate the sensitivity of present and future direct detection experiments to generalized neutrino interactions (GNI) with electrons through elastic neutrino-electron scattering. Using data from LUX-ZEPLIN, PandaX-4T, and XENONnT, we derive constraints on vector, axial-vector, scalar, and tensor effective couplings, and compare them with existing limits. Our results show that current xenon-based detectors already provide competitive bounds, with XENONnT offering the most stringent constraints due to its larger exposure and reduced backgrounds. Among the GNI couplings, the scalar contributions remain more weakly constrained, while tensor interactions yield the strongest limits. We also present projected sensitivities for the DARWIN experiment, showing potential improvements. These results demonstrate the capability of direct detection experiments, originally designed for dark matter searches, to provide complementary and competitive constraints on generalized neutrino interactions.
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de Montigny, M., Ouimet, P. P. A., Pinfold, J., Shaa, A., & Staelens, M. (2026). Minicharged particles at accelerators: progress and prospects. Eur. Phys. J.-Spec. Top., , 17pp.
Abstract: Minicharged particles (mCPs), hypothetical free particles with effective electric charges muchsmaller than the elementary charge,e, offer a valuable probe of dark sectors and fundamental physicsthrough several clear experimental signatures. Various models of physics beyond the Standard Modelpredict such particles, the existence of which could help elucidate the ongoing mysteries regarding electriccharge quantization and the nature of dark matter. Moreover, a hypothetical scenario involving a smallminicharged subcomponent of dark matter has recently been demonstrated as a viable explanation ofthe anomaly in the 21 cm hydrogen absorption signal reported by the EDGES collaboration. Althoughseveral decades of indirect observations and direct experimental searches for mCPs at particle acceleratorshave led to severe constraints, a substantial window of the mCP mass-mixing parameter space remainsunexplored at the energy frontier accessible to current state-of-the-art accelerators, such as the LargeHadron Collider (LHC). Consequently, mCPs have remained topical over the years, and new experimentalsearches at accelerators have been gaining interest. In this article, we review the theoretical frameworks inwhich mCPs emerge and their phenomenological implications, the current direct and indirect constraintson mCPs, and the present state of the ongoing and upcoming searches for mCPs at particle accelerators.
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Zhang, S. C., Lyu, W. T., Wang, G. Y., Ma, B. Q., & Wang, E. (2026). Search for the Low-Lying Excited Baryon Σ*(1/2-) through Process Λc+ →Λ K0 π+. Chin. Phys. Lett., 43(5), 050203–8pp.
Abstract: Motivated by recent BESIII measurements of the singly Cabibbo-suppressed processes Lambda c+->Lambda K+pi 0 and Lambda c+->Lambda KS0 pi+ , we investigate the process Lambda c+->Lambda K0 pi+ by taking into account the contribution from the low-lying excited baryon Sigma*(1/2-), dynamically generated via the S-wave pseudoscalar meson-octet baryon interaction, as well as from the intermediate resonances K*(892) and N (1535). Our model successfully reproduces the BESIII pi+K0 invariant mass distribution, and predicts a distinct cusp structure around 1.43 GeV in the pi+Lambda invariant mass distribution, which is associated with the predicted Sigma*(1/2-). Future high-precise measurements of this process at BESIII, Belle II, and the proposed Super Tau-Charm Facility experiments will be crucial for testing the existence of Sigma*(1/2-) and advancing our understanding of the light baryon spectrum.
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Orsoe, R., Meighen-Berger, S., Lazar, J., Prado, J., Mozun-Mateo, I., Rosted, A., et al. (2026). NuBench: An open benchmark for deep learning-based event reconstruction in neutrino telescopes. J. Instrum., 21(5), T05001–58pp.
Abstract: Neutrino telescopes are large-scale detectors designed to observe Cherenkov radiation produced from neutrino interactions in water or ice. They exist to identify extraterrestrial neutrino sources and to probe fundamental questions pertaining to the elusive neutrino itself. A central challenge common across neutrino telescopes is to solve a series of inverse problems known as event reconstruction, which seeks to resolve properties of the incident neutrino, based on the detected Cherenkov light. In recent times, significant efforts have been made in adapting advances from deep learning research to event reconstruction, as such techniques provide several benefits over traditional methods. While a large degree of similarity in reconstruction needs and low-level data exists, cross-experimental collaboration has been hindered by a lack of diverse open-source datasets for comparing methods. We present NuBench, an open benchmark for deep learning-based event reconstruction in neutrino telescopes. NuBench comprises seven large-scale simulated datasets containing nearly 130 million charged-and neutral-current muon-neutrino interactions spanning 10 GeV to 100 TeV, generated across six detector geometries inspired by existing and proposed experiments. These datasets provide pulse-and event-level information suitable for developing and comparing machine-learning reconstruction methods in both water and ice environments. Using NuBench, we evaluate four reconstruction algorithms – ParticleNeT and DynEdge, both actively used within the KM3NeT and IceCube collaborations, respectively, along with GRIT and DeepIce – on up to five core tasks: energy and direction reconstruction, topology classification, interaction vertex prediction, and inelasticity estimation. Datasets, predictions and model artifacts are available here: https://github.com /graphnet-team/NuBench.
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Martinez-Lopez, E., Fuster-Martinez, N., Boronat, M., Grudiev, A., Gimeno, B., Gonzalez-Iglesias, D., et al. (2026). RF design of 3 GHz SCDTL structures for ion beams in medical accelerators. Nucl. Eng. Technol., 58(8), 104361–11pp.
Abstract: Linear accelerators provide significant advantages for hadron therapy, including fast energy modulation and reduced activation compared to circular machines. Although Side-Coupled Drift Tube LINACs (SCDTLs) are commonly integrated into the injector designs of such accelerators due to their compactness and efficiency, a detailed and systematic radio-frequency (RF) design and optimization framework focusing on their electromagnetic characteristics, RF efficiency, and achievable accelerating gradients is notably absent in existing literature. This study introduces a thorough approach to the RF design and optimization of a 3 GHz SCDTL structure, presented as a representative study for ion acceleration in medical applications, based on standard design parameters for such systems. By carefully refining the geometry of both accelerating and side-coupling cavities, as well as fine-tuning the coupling system, the work achieves maximized effective shunt impedance and achievable acceleration voltage, while ensuring compliance with limits on the maximum surface electric field and the modified Poynting vector. The findings provide a clear pathway to balance compact design and RF efficiency, contributing to the advancement of practical and high-performance 3 GHz SCDTL implementations in hadron therapy LINACs.
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