Add to ORKGAbstract: The atmospheric neutrino is still an important tool in the study of neutrino physics. The uncer-tainty of the predicted atmospheric neutrino ux is caused by the uncertainties in the physical assumptions and in the calculation scheme. We discuss them quantitatively, and present the works to reduce them. The uncertainty related to the hadronic interaction model was discussed before, therefore, we mainly study other uncertainty sources than the hadronic interaction model here
Using the most recent PDFs and the cosmic ray spectrum, we evaluate the charm/bottom induced prompt ...
We evaluate the prompt atmospheric neutrino flux including nuclear correction and B hadron contribut...
Using the ``modified DPMJET-III'' model explained in the previous paper, we calculate the atmospheri...
Abstract: Starting from a survey of experimental measurements, we assign uncertainties to the two mo...
An evaluation of the principal uncertainties in the computation of neutrino fluxes produced in cosmi...
The next generation of large-volume neutrino telescopes will include low-energy subarrays which will...
An evaluation of the principal uncertainties in the computation of neutrino fluxes produced in cosmi...
High-energy neutrinos, arising from decays of mesons that were produced through the cosmic rays coll...
Effects on atmospheric prompt neutrino fluxes of present uncertainties affecting the nucleon composi...
We present a new one-dimensional calculation of low and intermediate energy atmospheric muon and neu...
It is well known that the correlation of atmospheric neutrinos and muons are simply correlated in th...
The detection of astrophysical neutrinos, certainly a break-through result, introduced new experimen...
Email of contact person Abstract: Finding neutrinos of astrophysical origin requires a good understa...
We will present the strategy to refurbish a simulation code ATMNC developed by M. Honda which provid...
Neutrinos produced by cosmic ray interactions in the Earth's atmosphere have proven to be an invalua...
Using the most recent PDFs and the cosmic ray spectrum, we evaluate the charm/bottom induced prompt ...
We evaluate the prompt atmospheric neutrino flux including nuclear correction and B hadron contribut...
Using the ``modified DPMJET-III'' model explained in the previous paper, we calculate the atmospheri...
Abstract: Starting from a survey of experimental measurements, we assign uncertainties to the two mo...
An evaluation of the principal uncertainties in the computation of neutrino fluxes produced in cosmi...
The next generation of large-volume neutrino telescopes will include low-energy subarrays which will...
An evaluation of the principal uncertainties in the computation of neutrino fluxes produced in cosmi...
High-energy neutrinos, arising from decays of mesons that were produced through the cosmic rays coll...
Effects on atmospheric prompt neutrino fluxes of present uncertainties affecting the nucleon composi...
We present a new one-dimensional calculation of low and intermediate energy atmospheric muon and neu...
It is well known that the correlation of atmospheric neutrinos and muons are simply correlated in th...
The detection of astrophysical neutrinos, certainly a break-through result, introduced new experimen...
Email of contact person Abstract: Finding neutrinos of astrophysical origin requires a good understa...
We will present the strategy to refurbish a simulation code ATMNC developed by M. Honda which provid...
Neutrinos produced by cosmic ray interactions in the Earth's atmosphere have proven to be an invalua...
Using the most recent PDFs and the cosmic ray spectrum, we evaluate the charm/bottom induced prompt ...
We evaluate the prompt atmospheric neutrino flux including nuclear correction and B hadron contribut...
Using the ``modified DPMJET-III'' model explained in the previous paper, we calculate the atmospheri...