Dark matter raining on DUNE and other large volume detectors

• DOI: 10.1007/jhep11(2024)011
• Publication Date: 2024-11-06T11:06:25Z
• Authors: Javier F. Acevedo; Joshua Berger; Peter B. Denton
• Keywords: New Light Particles; High Energy Astrophysical Phenomena (astro-ph.HE); FOS: Physical sciences; QC770-798; 01 natural sciences; High Energy Physics - Experiment; High Energy Physics - Phenomenology; High Energy Physics - Experiment (hep-ex); High Energy Physics - Phenomenology (hep-ph); Nuclear and particle physics. Atomic energy. Radioactivity; 0103 physical sciences; Models for Dark Matter; Astrophysics - High Energy Astrophysical Phenomena; Specific BSM Phenomenology; Particle Nature of Dark Matter

Abstract

Direct detection is a powerful means of searching for particle physics evidence of dark matter (DM) heavier than about a GeV with 𝒪(kiloton) volume, low-threshold detectors. In many scenarios, some fraction of the DM may be boosted to large velocities enhancing and generally modifying possible detection signatures. We investigate the scenario where 100% of the DM is boosted at the Earth due to new attractive long-range forces. This leads to two main improvements in detection capabilities: (1) the large boost allows for detectable signatures of DM well below a GeV at large-volume neutrino detectors, such as DUNE, Super-K, Hyper-K, and JUNO, as possible DM detectors, and (2) the flux at the Earth’s surface is enhanced by a focusing effect. In addition, the model leads to a significant anisotropy in the signal with the DM flowing dominantly vertically at the Earth’s surface instead of the typical approximately isotropic DM signal. We develop the theory behind this model and also calculate realistic constraints using a detailed GENIE simulation of the signal inside detectors.