Zobrazeno 1 - 10
of 21
pro vyhledávání: '"T. S. Sinegovskaya"'
Publikováno v:
Physics of Particles and Nuclei Letters. 20:27-37
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0e688fd01d97126deb0908cc0c1b2fbe
https://doi.org/10.1134/s1547477123010090
https://doi.org/10.1134/s1547477123010090
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 85:433-437
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-Kamiokande experiments. Atmospheric neutrino spectra are calculated with a ce
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7fdd55f8f560ff925ab811752f1f90d8
https://doi.org/10.3103/s1062873821040195
https://doi.org/10.3103/s1062873821040195
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 83:933-936
The atmospheric muon and neutrino fluxes at energies from 10 GeV to 10 PeV are calculated with the Kimel–Mokhov (KM), SIBYLL 2.1, EPOS LHC, and QGSJET-II hadronic models for known parameterizations of the cosmic ray spectra by Zatsepin--Sokolskaya
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c17940e30387f49511a4c84ff74ec06a
https://doi.org/10.3103/s1062873819080203
https://doi.org/10.3103/s1062873819080203
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 81:516-519
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 two experimentally based Zatsepin–Sokol’skaya and H
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::61747b1554c4faa3660eccdd24e5f496
https://doi.org/10.3103/s1062873817040323
https://doi.org/10.3103/s1062873817040323
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::932041db8d614087727fc8206924ee17
http://arxiv.org/abs/1907.00640
http://arxiv.org/abs/1907.00640
Publikováno v:
Journal of Experimental and Theoretical Physics. 116:395-413
We present the calculations of the atmospheric muon fluxes at energies 10–107 GeV based on a numerical-analytical method for solving the hadron-nucleus cascade equations. It allows the non-power-law behavior of the primary cosmic ray (PCR) spectrum
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::400e307cadc6e9f29089448987e9e1f5
https://doi.org/10.1134/s1063776113020143
https://doi.org/10.1134/s1063776113020143
Publikováno v:
International Journal of Modern Physics A. 25:3733-3740
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::36ffa765d8e21bc9b182f436ae53990e
https://doi.org/10.1142/s0217751x10049748
https://doi.org/10.1142/s0217751x10049748
Publikováno v:
Physics of Atomic Nuclei. 70:1913-1925
A new calculation of the atmospheric fluxes of cosmic-ray hadrons and muons in the energy range 10–104 GeV is performed on the basis of the method for solving nuclear-cascade equations with allowance for a nonscaling behavior of inclusive hadron-pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0724c0e25d3258453487f0453d7b85a7
https://doi.org/10.1134/s1063778807110117
https://doi.org/10.1134/s1063778807110117
Publikováno v:
Russian Physics Journal. 50:891-897
New results of calculations of nucleon, π-and K-meson, and muon fluxes generated during high energy cosmic ray interactions with the Earth’s atmosphere are presented. The calculations are based on the method of solving the nuclear cascade equation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::339c650ea9512ac4f4ec1e344c1b663a
https://doi.org/10.1007/s11182-007-0130-4
https://doi.org/10.1007/s11182-007-0130-4
Publikováno v:
Physical Review D. 91
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::970673aabdcff62b8695deec2ad4a1b7
https://doi.org/10.1103/physrevd.91.063011
https://doi.org/10.1103/physrevd.91.063011