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Probing Cosmic-Ray Accelerated Light Dark Matter with IceCube

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arxiv 2004.03161 v2 pith:E6PRW2RQ submitted 2020-04-07 astro-ph.HE hep-exhep-ph

classification astro-ph.HEhep-exhep-ph
keywords high-energycross-sectiondarkdetectiondirectdm-nucleonenergyicecube
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

The direct detection of particle dark matter through its scattering with nucleons is of fundamental importance to understand the nature of DM. In this work, we propose that the high-energy neutrino detectors like IceCube can be used to uniquely probe the DM-nucleon cross-section for high-energy DM of $\sim$ PeV, up-scattered by the high-energy cosmic rays. We derive for the first time strong constraints on the DM-nucleon cross-section down to $\sim 10^{-32}$ cm$^2$ at this energy scale for sub-GeV DM candidates. Such independent probe at energy scale far exceeding other existing direct detection experiments can therefore provide useful insights complementary to other searches.

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  1. Dark Photons and Gravitino Like Particles: Complete EFT Operator Basis

    hep-ph 2024-12 conditional novelty 6.0 of 10

    A new on-shell method using Young tableaux constructs complete EFT operator bases for massive particles of any spin, applied to dark photons and spin-3/2 gravitino-like particles up to dimension 8.

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