activity
20242026
collaborators

26 papers

hep-ex2026

Constraints on Sub-MeV Dark Matter from Solar Reflection with DAMIC-M

K. Aggarwal, I. Arnquist, N. Avalos +41

The Sun acts as a natural dark matter accelerator. Galactic halo particles scattering in the solar plasma emerge with velocities well beyond the Galactic escape speed, providing a…

physics.ins-det2026

Model-independent searches of new physics in DARWIN with a semi-supervised deep learning pipeline

J. Aalbers, K. Abe, M. Adrover +231

We present a novel deep learning pipeline to perform a model-independent, likelihood-free search for anomalous (i.e., non-background) events in the proposed next generation multi-t…

astro-ph.HE2026

Sensitivity of the As-Built Askaryan Radio Array to Ultra-High Energy Neutrinos

ARA Collaboration, N. Alden, S. Ali +71

The Askaryan Radio Array (ARA) is an ultra-high energy (UHE) neutrino observatory designed to detect the impulsive radio waves produced by relativistic particle cascades in the Ant…

physics.ins-det2026

Low-Energy Nuclear Recoil Calibration of XENONnT with a YBe Photoneutron Source

XENON Collaboration, E. Aprile, J. Aalbers +169

Characterizing low-energy, keV-range nuclear recoils near the detector threshold is one of the major challenges for large direct dark matter detectors. To that end, we have success…

astro-ph.HE2026

Observation of In-ice Askaryan Radiation from High-Energy Cosmic Rays

ARA Collaboration, N. Alden, S. Ali +74

We present the first experimental evidence for in-ice Askaryan radiation -- coherent charge-excess radio emission -- from high-energy particle cascades developing in the Antarctic…

astro-ph.IM2026

Modeling the refractive index profile n(z) of polar ice for ultra-high energy neutrino experiments

S. Ali, P. Allison, S. Archambault +67

We have developed an in-situ index of refraction profile n(z) for cold polar ice, using the transit times of radio signals broadcast from an englacial transmitter to 2-5 km distant…