Add to ORKGThe result of a new calculation of the atmospheric muon and neutrino fluxes and the energy spectrum of muon-neutrinos produced in individual extensive air showers (EAS) initiated by proton and gamma-ray primaries is reported. Also explained is the possibility of detecting atmospheric nu sub mu's due to gamma-rays from these sources
We present a new one-dimensional calculation of low and intermediate energy atmospheric muon and neu...
The first generation of large and precise detectors, some initially dedicated to search for nucleon ...
Muons produced in atmospheric cosmic ray showers account for the by far dominant part of the event y...
Some aspects of neutrino astronomy are illustrated by calculating the neutrino-induced muon flux fro...
This paper is a mini-review of the atmospheric muon and neutrino flux calculations based upon a rece...
In this talk I review measurements and calculations of the flux of neutrinos produced by interaction...
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...
We obtain the horizontal air shower rate from the (EeV) high energy neutrino flux predicted in some ...
This talk reports the latest indications of an anomaly in the measurements of atmospheric neutrinos....
The result of a calculation of the expected number of muons in gamma ray initiated and cosmic ray in...
In the TeV energy region and above, the uncertainty in the level of prompt atmospheric neutrinos wou...
The atmospheric neutrino flux has been measured by several experiments and its understanding has bee...
This paper is a brief overview of the theory and experimental data of atmospheric neutrino productio...
Focusing on high energy neutrinos ( or = 1 TeV), a new calculation of atmospheric neutrino intensiti...
We present a new one-dimensional calculation of low and intermediate energy atmospheric muon and neu...
The first generation of large and precise detectors, some initially dedicated to search for nucleon ...
Muons produced in atmospheric cosmic ray showers account for the by far dominant part of the event y...
Some aspects of neutrino astronomy are illustrated by calculating the neutrino-induced muon flux fro...
This paper is a mini-review of the atmospheric muon and neutrino flux calculations based upon a rece...
In this talk I review measurements and calculations of the flux of neutrinos produced by interaction...
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...
We obtain the horizontal air shower rate from the (EeV) high energy neutrino flux predicted in some ...
This talk reports the latest indications of an anomaly in the measurements of atmospheric neutrinos....
The result of a calculation of the expected number of muons in gamma ray initiated and cosmic ray in...
In the TeV energy region and above, the uncertainty in the level of prompt atmospheric neutrinos wou...
The atmospheric neutrino flux has been measured by several experiments and its understanding has bee...
This paper is a brief overview of the theory and experimental data of atmospheric neutrino productio...
Focusing on high energy neutrinos ( or = 1 TeV), a new calculation of atmospheric neutrino intensiti...
We present a new one-dimensional calculation of low and intermediate energy atmospheric muon and neu...
The first generation of large and precise detectors, some initially dedicated to search for nucleon ...
Muons produced in atmospheric cosmic ray showers account for the by far dominant part of the event y...