Effects on atmospheric prompt neutrino fluxes of present uncertainties affecting the nucleon composition are studied by using the PROSA fit to parton distribution functions (PDFs). The PROSA fit extends the precision of the PDFs to low x, which is the kinematic region of relevance for high-energy neutrino production, by taking into account LHCb data on charm and bottom hadroproduction. In the range of neutrino energies explored by present Very Large Volume Neutrino Telescopes, it is found that PDF uncertainties are far smaller with respect to those due to renormalization and factorization scale variation and to assumptions on the cosmic ray composition, which at present dominate and limit our knowledge of prompt neutrino fluxes. A discussio...
The composition in terms of nuclear species of the primary cosmic ray flux is largely uncertain in t...
Abstract The high-energy atmospheric neutrino flux is dominated by neutrinos from the decays of char...
Using the most recent PDFs and the cosmic ray spectrum, we evaluate the charm/bottom induced prompt ...
Effects on atmospheric prompt neutrino fluxes of present uncertainties affecting the nucleon composi...
The recent observation of very high energy cosmic neutrinos by IceCube heralds the beginning of neut...
The next generation of large-volume neutrino telescopes will include low-energy subarrays which will...
We re-evaluate the prompt atmospheric neutrino flux, using the measured charm cross sections at RHIC...
An evaluation of the principal uncertainties in the computation of neutrino fluxes produced in cosmi...
We evaluate the prompt atmospheric neutrino flux at high energies using three different frameworks f...
We evaluate the prompt atmospheric neutrino flux including nuclear correction and B hadron contribut...
The composition in terms of nuclear species of the primary cosmic ray flux is largely uncertain in t...
Abstract: Starting from a survey of experimental measurements, we assign uncertainties to the two mo...
High-energy neutrinos, arising from decays of mesons that were produced through the cosmic rays coll...
The IceCube Neutrino Observatory is a cubic kilometre scale detector for high-energy neutrinos above...
The composition in terms of nuclear species of the primary cosmic ray flux is largely uncertain in t...
Abstract The high-energy atmospheric neutrino flux is dominated by neutrinos from the decays of char...
Using the most recent PDFs and the cosmic ray spectrum, we evaluate the charm/bottom induced prompt ...
Effects on atmospheric prompt neutrino fluxes of present uncertainties affecting the nucleon composi...
The recent observation of very high energy cosmic neutrinos by IceCube heralds the beginning of neut...
The next generation of large-volume neutrino telescopes will include low-energy subarrays which will...
We re-evaluate the prompt atmospheric neutrino flux, using the measured charm cross sections at RHIC...
An evaluation of the principal uncertainties in the computation of neutrino fluxes produced in cosmi...
We evaluate the prompt atmospheric neutrino flux at high energies using three different frameworks f...
We evaluate the prompt atmospheric neutrino flux including nuclear correction and B hadron contribut...
The composition in terms of nuclear species of the primary cosmic ray flux is largely uncertain in t...
Abstract: Starting from a survey of experimental measurements, we assign uncertainties to the two mo...
High-energy neutrinos, arising from decays of mesons that were produced through the cosmic rays coll...
The IceCube Neutrino Observatory is a cubic kilometre scale detector for high-energy neutrinos above...
The composition in terms of nuclear species of the primary cosmic ray flux is largely uncertain in t...
Abstract The high-energy atmospheric neutrino flux is dominated by neutrinos from the decays of char...
Using the most recent PDFs and the cosmic ray spectrum, we evaluate the charm/bottom induced prompt ...