Investigating light neutralinos at neutrino telescopes
V. Niro, A. Bottino, N. Fornengo, and S. Scopel

TL;DR
This paper analyzes the potential for neutrino telescopes to detect light neutralinos, considering various uncertainties and their relation to DAMA/LIBRA data, to improve understanding of dark matter properties.
Contribution
It provides a detailed evaluation of neutrino signals from light neutralinos in an effective MSSM model, incorporating uncertainties and neutrino oscillations, and links to DAMA/LIBRA results.
Findings
Identifies neutralino mass ranges detectable by neutrino telescopes.
Shows how combining neutrino data with DAMA/LIBRA can constrain dark matter properties.
Highlights the importance of astrophysics and particle physics uncertainties in detection prospects.
Abstract
We present a detailed analysis of the neutrino-induced muon signals coming from neutralino pair-annihilations inside the Sun and the Earth with particular emphasis for light neutralinos. The theoretical model considered is an effective MSSM without gaugino-mass unification, which allows neutralinos of light masses (below 50 GeV). The muon events are divided in through-going and stopping muons, using the geometry of the Super-Kamiokande detector. In the evaluation of the signals, we take into account the relevant hadronic and astrophysics uncertainties and include neutrino oscillation and propagation properties in a consistent way. We derive the ranges of neutralino masses which could be explored at neutrino telescopes with a low muon-energy threshold (around 1 GeV) depending on the category of events and on the values of the various astrophysics and particle-physics parameters. A final…
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