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arXiv · 1602.08441

Prompt neutrino flux in the atmosphere revisited

M. V. Garzelli·S. Moch·G. Sigl
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Abstract

Prompt neutrino fluxes due to the interactions of high-energy cosmic rays with the Earth's atmosphere are backgrounds in the search for high-energy neutrinos of galactic or extra-galactic origin performed by Very Large Volume Neutrino Telescopes. We summarize our predictions for prompt neutrinos, showing their basic features as emerging from the calculation in a QCD framework capable of describing recent charm data from the Large Hadron Collider.

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M. V. Garzelli, S. Moch, G. Sigl. 2016-02-26. Prompt neutrino flux in the atmosphere revisited. https://arxiv.org/abs/1602.08441

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