Zobrazeno 1 - 10
of 65
pro vyhledávání: '"Sinegovsky, S. I"'
Statistical analysis is performed of the atmospheric neutrino flux models as compared with the data of Frejus, AMANDA-II, IceCube, ANTARES, and Super-Kamiokande experiments. The analysis enables the evaluation of the confidence level of the flux mode
Externí odkaz:
http://arxiv.org/abs/2109.13000
Publikováno v:
Journal of Physics: Conf. Series. 2019. V. 1181, 012054
Recently the atmospheric muon spectra at high energies were reconstructed for two ranges of zenith angles, basing on the events collected with the IceCube detector. These measurements reach high energies at which the contribution to atmospheric muon
Externí odkaz:
http://arxiv.org/abs/1907.00640
Autor:
Sinegovsky, S. I., Sorokovikov, M. N.
Publikováno v:
European Physical Journal C volume 80, Article number: 34 (2020)
We calculate the atmospheric flux of prompt neutrinos, produced in decays of the charmed particles at energies beyond 1 TeV. Cross sections of the $D$-mesons and ${\Lambda}^{+}_{c}$ baryons production in pA and $\pi$A collisions are calculated in the
Externí odkaz:
http://arxiv.org/abs/1812.11341
Publikováno v:
Phys. Rev. D 91, 063011 (2015)
We calculate the atmospheric neutrino fluxes in the energy range $100$ GeV -- $10$ PeV with the use of several known hadronic models and a few parametrizations of the cosmic ray spectra which take into account the knee. The calculations are compared
Externí odkaz:
http://arxiv.org/abs/1407.3591
High-energy neutrinos from decays of mesons, produced in collisions of cosmic ray particles with air nuclei, form unavoidable background for detection of astrophysical neutrinos. More precise calculations of the high-energy neutrino spectrum are requ
Externí odkaz:
http://arxiv.org/abs/1306.5907
High-energy neutrinos, arising from decays of mesons produced through the collisions of cosmic ray particles with air nuclei, form the background in the astrophysical neutrino detection problem. An ambiguity in high-energy behavior of pion and especi
Externí odkaz:
http://arxiv.org/abs/1109.3576
Autor:
Al-Rubaiee, A. A., Gress, O. A., Kochanov, A. A., Lokhtin, K. S., Parfenov, Y. V., Sinegovsky, S. I
The simulation of the Cherenkov light lateral distribution function (LDF) in Extensive Air Showers (EAS) was perfomed with the CORSIKA code in the energy range 10^13-10^16 eV for configuration of the Tunka-25 EAS array. On the basis of this simulatio
Externí odkaz:
http://arxiv.org/abs/1104.2510
High-energy neutrinos, arising from decays of mesons that were produced through the cosmic rays collisions with air nuclei, form unavoidable background noise in the astrophysical neutrino detection problem. The atmospheric neutrino flux above 1 PeV s
Externí odkaz:
http://arxiv.org/abs/1010.2336
Publikováno v:
Int.J.Mod.Phys.A25:3733-3740,2010
In the near future the energy region above few hundreds of TeV may really be accessible for measurements of the atmospheric muon spectrum by the IceCube array. Therefore one expects that muon flux uncertainties above 50 TeV, related to a poor knowled
Externí odkaz:
http://arxiv.org/abs/0906.3791
We study the influence of hadron interaction features on the high-energy atmospheric neutrino spectrum. The 1D calculation is performed with use of the known high-energy hadronic models, SIBYLL 2.1, QGSJET-II, Kimel and Mokhov, for the parameterizati
Externí odkaz:
http://arxiv.org/abs/0906.0671