Corpus ID: 237940992

High-energy spectra of the atmospheric neutrinos: predictions and measurements

@inproceedings{Kochanov2021HighenergySO,
  title={High-energy spectra of the atmospheric neutrinos: predictions and measurements},
  author={Aleksey Kochanov and Anna Morozova and T. S. Sinegovskaya and Supa School of Physics and U. SBRussianAcademyofSciencesIrkutskStateU.IrkutskSta},
  year={2021}
}
  • A. Kochanov, A. Morozova, +2 authors U. SBRussianAcademyofSciencesIrkutskStateU.IrkutskSta
  • Published 27 September 2021
  • Physics
A. A. Kochanov, ∗ A. D. Morozova, 2 T. S. Sinegovskaya, and S. I. Sinegovsky 3, † Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences, RU-664033, Irkutsk, Russia Irkutsk State University, RU-664003 Irkutsk, Russia Dzhelepov Laboratory of Nuclear Problems, Joint Institute for Nuclear Research, RU-141980 Dubna, Russia Irkutsk State Transport University, RU-664074, Irkutsk, Russia (Dated: September 28, 2021) 

Figures and Tables from this paper

References

SHOWING 1-10 OF 80 REFERENCES
Calculation of atmospheric high-energy neutrino spectra and the measurement data of IceCube and ANTARES experiments
Presented are results of calculation of the atmospheric neutrino spectra in the energy range from 100 GeV to 10 PeV using the QGSJET-II and SIBYLL 2.1 models of hadron–nuclear interactions and twoExpand
Influence of hadronic interaction models on characteristics of the high-energy atmospheric neutrino flux
The high-energy conventional atmospheric neutrino fluxes are calculated with the hadronic interaction models: Kimel & Mokhov, QGSJET II-03(04), SIBYL 2.1(2.3), EPOS LHC. The influence ofExpand
Atmospheric Neutrino Spectra: A Statistical Analysis of Calculations in Comparison with Experiment
Abstract A statistical analysis is performed to compare calculated spectra of atmospheric neutrinos and measuring data obtained in the Frejus, AMANDA-II, IceCube, ANTARES, and Super-KamiokandeExpand
The comparison of the calculated atmospheric neutrino spectra with the measurements of IceCube and ANTARES experiments
We calculate the atmospheric neutrino spectra in the energy range of 102 − 107 GeV using the hadronic models QGSJET-II, SIBYLL 2.1 and the parameterizations of cosmic ray spectra byExpand
The energy spectrum of atmospheric neutrinos between 2 and 200 TeV with the AMANDA-II detector
The muon and anti-muon neutrino energy spectrum is determined from 2000-2003 AMANDA telescope data using regularised unfolding. This is the first measurement of atmospheric neutrinos in the energyExpand
Measurement of the atmospheric νe flux in IceCube.
TLDR
This constitutes the first observation of electron neutrinos and neutral current interactions in a very large volume neutrino telescope optimized for the TeV energy range. Expand
Improvement of low energy atmospheric neutrino flux calculation using the JAM nuclear interaction model
We present the calculation of the atmospheric neutrino fluxes with an interaction model named JAM, which is used in PHITS (Particle and Heavy-Ion Transport code System) [K. Niita et al., RadiationExpand
PHENOMENOLOGY OF ATMOSPHERIC NEUTRINOS a
The relevance of the data concerning upward–going muons for the solution of the atmospheric neutrino problem is stressed. In particular, their inclusion in the analysis confirms the goodness of theExpand
Prompt neutrinos from atmospheric charm in the general-mass variable-flavor-number scheme
A bstractWe 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,Expand
Measurement of the atmospheric νμ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope
Atmospheric neutrinos are produced during cascades initiated by the interaction of primary cosmic rays with air nuclei. In this paper, a measurement of the atmospheric $\nu_{\mu} + \bar{\nu}_{\mu}$Expand
...
1
2
3
4
5
...