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Prompt neutrinos from atmospheric charm in the general-mass variable-flavor-number scheme
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We present predictions for the prompt-neutrino flux arising from the decay of charmed mesons and baryons produced by the interactions of high-energy cosmic rays in the Earth's atmosphere, making use of a QCD approach on the basis of the general-mass variable-flavor-number scheme for the description of charm hadroproduction at NLO, complemented by a consistent set of fragmentation functions. We compare the theoretical results to those already obtained by our and other groups with different theoretical approaches. We provide comparisons with the experimental results obtained by the IceCube Collaboration in two different analyses and we discuss the implications for parton distribution functions.
Forward citations
Cited by 2 Pith papers
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Differential cross-section measurements of $D^{\pm}$ and $D_{s}^{\pm}$ meson production in proton-proton collisions at $\sqrt{s} = 13$ TeV with the ATLAS detector
ATLAS reports the first differential D_s± meson cross-section measurement and extends D±/D_s± data to pT = 100 GeV at 13 TeV, finding consistency with NLO QCD within uncertainties.
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Charm production and hadronisation in pp and p--Pb collisions at $\sqrt{s_{\rm NN}} = $ 5.02 TeV at the LHC with ALICE
A proceedings summary of already published ALICE charm production measurements in pp and p-Pb collisions, with no new data or analysis.
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