Search for U(1) charged Dark Matter with neutrino telescope
arXiv:2011.03165 · doi:10.1007/JHEP03(2021)047
Abstract
We study a simple Dirac fermion dark matter model in U(1) theory. The new light gauge boson plays important roles in both dark matter physics and the explanation for the muon anomaly. The observed dark matter relic density is realized by a large U(1) charge without introducing a resonance effect of the boson. As a by-product of the model, characteristic neutrino signatures from sub-GeV dark matter are predicted depending on the mass spectrum. We formulate the analysis of , and of followed by , in a model independent way. The energy spectrum of neutrinos in the former process is monochromatic while in the latter process is bowl-shape. We also evaluate sensitivity at Super-Kamiokande and future Hyper-Kamiokande detectors. The analysis is finally applied to the U(1) dark matter model.
32 pages, 6 figures; v2: added references and comments, corrected the neutrino spectrum from secluded annihilation and corresponding plots, conclusion unchanged, version to be published in JHEP
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