no code implementations • 9 Mar 2021 • Victor P. Goncalves, Rafal Maciula, Antoni Szczurek
The predictions for the atmospheric neutrino flux at high energies strongly depend on the contribution of prompt neutrinos, which are determined by the production of charmed meson in the atmosphere at very forward rapidities.
High Energy Physics - Phenomenology High Energy Physics - Experiment
no code implementations • 11 Dec 2020 • Rafal Maciula
We discuss cross sections for $\nu_{\tau}$ and ${\overline \nu}_{\tau}$ production from the direct $D_s^{\pm} \to \nu_{\tau}/{\overline \nu}_{\tau}$ and chain $D_s^{\pm} \to \tau^+/\tau^- \to \nu_{\tau}/{\overline \nu}_{\tau}$ decays in $p\!+^{96}\!\mathrm{Mo}$ scattering with proton beam $E_{\mathrm{lab}}$ = 400 GeV \textit{i. e.} at $\sqrt{s}_{NN}$ = 27. 4 GeV.
High Energy Physics - Phenomenology
