Add to ORKGWe evaluate the prompt atmospheric neutrino flux including nuclear correction and B hadron contribution in the different frameworks: NLO perturbative QCD and dipole models. The nuclear effect is larger in the prompt neutrino flux than in the total charm production cross section, and it reduces the fluxes by 10%−30% depending on the model. We also investigate the uncertainty using the QCD scales allowed by the charm cross section data from RHIC and LHC experiments
The IceCube Neutrino Observatory is a cubic kilometre scale detector for high-energy neutrinos above...
Abstract The high-energy atmospheric neutrino flux is dominated by neutrinos from the decays of char...
We present predictions for the prompt-neutrino flux arising from the decay of charmed mesons and bar...
We evaluate the prompt atmospheric neutrino flux including nuclear correction and B hadron contribut...
We evaluate the prompt atmospheric neutrino flux at high energies using three different frameworks f...
Using the most recent PDFs and the cosmic ray spectrum, we evaluate the charm/bottom induced prompt ...
We evaluate the prompt atmospheric neutrino flux using the different QCD models for heavy quark prod...
We re-evaluate the prompt atmospheric neutrino flux, using the measured charm cross sections at RHIC...
The recent observation of very high energy cosmic neutrinos by IceCube heralds the beginning of neut...
Prompt neutrinos due to the decay of charmed mesons produced in the atmosphere from cosmic-ray and a...
High-energy neutrinos, arising from decays of mesons that were produced through the cosmic rays coll...
We calculate the atmospheric flux of prompt neutrinos, produced in decays of the charmed particles a...
Prompt neutrino fluxes are basic backgrounds in the search of high-energy neutrinos of astrophysical...
The predictions for the atmospheric neutrino flux at high energies strongly depend on the contributi...
We improve the accuracy of the extrapolation of the gluon distribution of the proton to very small x...
The IceCube Neutrino Observatory is a cubic kilometre scale detector for high-energy neutrinos above...
Abstract The high-energy atmospheric neutrino flux is dominated by neutrinos from the decays of char...
We present predictions for the prompt-neutrino flux arising from the decay of charmed mesons and bar...
We evaluate the prompt atmospheric neutrino flux including nuclear correction and B hadron contribut...
We evaluate the prompt atmospheric neutrino flux at high energies using three different frameworks f...
Using the most recent PDFs and the cosmic ray spectrum, we evaluate the charm/bottom induced prompt ...
We evaluate the prompt atmospheric neutrino flux using the different QCD models for heavy quark prod...
We re-evaluate the prompt atmospheric neutrino flux, using the measured charm cross sections at RHIC...
The recent observation of very high energy cosmic neutrinos by IceCube heralds the beginning of neut...
Prompt neutrinos due to the decay of charmed mesons produced in the atmosphere from cosmic-ray and a...
High-energy neutrinos, arising from decays of mesons that were produced through the cosmic rays coll...
We calculate the atmospheric flux of prompt neutrinos, produced in decays of the charmed particles a...
Prompt neutrino fluxes are basic backgrounds in the search of high-energy neutrinos of astrophysical...
The predictions for the atmospheric neutrino flux at high energies strongly depend on the contributi...
We improve the accuracy of the extrapolation of the gluon distribution of the proton to very small x...
The IceCube Neutrino Observatory is a cubic kilometre scale detector for high-energy neutrinos above...
Abstract The high-energy atmospheric neutrino flux is dominated by neutrinos from the decays of char...
We present predictions for the prompt-neutrino flux arising from the decay of charmed mesons and bar...