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arxiv: 1206.5530 · v2 · submitted 2012-06-24 · 🌌 astro-ph.IM · astro-ph.HE· physics.ins-det

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Calculation of the Cherenkov light yield from low energetic secondary particles accompanying high-energy muons in ice and water with Geant 4 simulations

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classification 🌌 astro-ph.IM astro-ph.HEphysics.ins-det
keywords distributionenergyangularcherenkovparticlessecondarycalculationinvestigate
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In this work we investigate and parameterize the amount and angular distribution of Cherenkov photons, which are generated by low-energy secondary particles (typically $\lesssim 500 $\,MeV), which accompany a muon track in water or ice. These secondary particles originate from small energy loss processes. We investigate the contributions of the different energy loss processes as a function of the muon energy and the maximum transferred energy. For the calculation of the angular distribution we have developed a generic transformation method, which allows us to derive the angular distribution of Cherenkov photons for an arbitrary distribution of track directions and their velocities.

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Cited by 1 Pith paper

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  1. POLARIS: A Sparse Radial Neutrino Telescope Design for the Pacific Ocean

    astro-ph.HE 2026-04 unverdicted novelty 6.0

    POLARIS is a radial sparse Cherenkov detector that targets the natural horizontal geometry of ultra-high-energy neutrino-induced muons to reach PeV sensitivities with only 1100 modules.