Extending the Dark Matter Reach of Water Cherenkov Detectors using Jupiter

Abstract

We propose the first method for water Cherenkov detectors to constrain GeV-scale dark matter (DM) below the solar evaporation mass. While previous efforts have highlighted the Sun and Earth as DM capture targets, we demonstrate that Jupiter is a viable target. Jupiter's unique characteristics, such as its lower core temperature and significant gravitational potential, allow it to capture and retain light DM more effectively than the Sun, particularly in the mass range below 4 GeV where direct detection sensitivity diminishes. Our calculations provide the first sensitivity estimates to GeV-scale annihilating DM within Jupiter, predicting Hyper-K can reach spin dependent cross sections as low as ${\sigma }_{p\chi }^{\mathrm{SD}}=2\times 10^{-35}{\mathrm{cm}}^2$ for DM masses below 2 GeV. This surpasses current solar limits and direct detection results. We additionally provide estimates for Super-K ORCA, and the IceCube-Upgrade, showing that these experiments could provide complimentary bounds to direct detection experiments.

10 pages, 5 figures, 1 appendix. Discussion extended, matches published version

References in corpus (29)

• First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
• Dark Matter Search Results from the PandaX-4T Commissioning Run
• Dark Matter Search Results from the Complete Exposure of the PICO-60 C${}_3$F${}_8$ Bubble Chamber
• Towards Closing the Window on Strongly Interacting Dark Matter: Far-Reaching Constraints from Earth's Heat Flow
• Improvement of low energy atmospheric neutrino flux calculation using the JAM nuclear interaction model
• Dark Matter Search Results from 4.2 Tonne-Years of Exposure of the LUX-ZEPLIN (LZ) Experiment
• Spin-Dependent Weakly-Interacting-Massive-Particle--Nucleon Cross Section Limits from First Data of PandaX-II Experiment
• Final Results of the PICASSO Dark Matter Search Experiment
• Search for Coherent Elastic Scattering of Solar ${}^8$B Neutrinos in the XENON1T Dark Matter Experiment
• Neutrino-Nucleon Cross-Section Model Tuning in GENIE v3
• Measurement of the Atmospheric ${\nu }_e$ flux in IceCube
• The New DAMA Dark-Matter Window and Energetic-Neutrino Searches
• Characterization of the Astrophysical Diffuse Neutrino Flux using Starting Track Events in IceCube
• Evaporation of dark matter from celestial bodies
• Enhancing Dark Matter Annihilation into Neutrinos
• Search for GeV-scale Dark Matter Annihilation in the Sun with IceCube DeepCore
• Testing spin-dependent dark matter interactions with lithium aluminate targets in CRESST-III
• Graph Neural Networks for Low-Energy Event Classification & Reconstruction in IceCube
• Planet-bound dark matter and the internal heat of Uranus, Neptune, and hot-Jupiter exoplanets
• Jupiter missions as probes of dark matter
• Light mass window of lepton portal dark matter
• $\chi$aro$\nu$: a tool for neutrino flux generation from WIMPs
• Light lepton portal dark matter meets the LHC
• Simulation of energy transport by dark matter scattering in stars
• Upgrading the COSINE-100 Experiment for Enhanced Sensitivity to Low-Mass Dark Matter Detection
• Search for Light Dark Matter with NEWS-G at the Laboratoire Souterrain de Modane Using a Methane Target
• Monoenergetic Neutrinos from WIMP Annihilation in Jupiter
• First Detailed Calculation of Atmospheric Neutrino Foregrounds to the Diffuse Supernova Neutrino Background in Super-Kamiokande
• KM3NeT upper bounds of detection rates of solar neutrinos from annihilations of dark matter at the solar core

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