activity
19992020
most citedThe spectrum features of UHECRs below and surrounding GZK

73 citations · 126 across the 7 of their papers we have counts for

collaborators

7 papers

physics.ins-det2020★ 18 cited

SND@LHC

SHiP Collaboration, C. Ahdida, A. Akmete +341

We propose to build and operate a detector that, for the first time, will measure the process at the LHC and search for feebly interacting particles (FIPs) in an unexplor…

astro-ph2004

Characteristics of EAS and Primary Particle Mass Composition in the Energy Region of eV by Yakutsk Data

S. P. Knurenko, V. P. Egorova, A. A. Ivanov +5

In the work the data of the Yakutsk complex EAS array and their comparison with calculation in the case of primary nuclei of different chemical elements are presented. The calculat…

astro-ph2004★ 7 cited

Fluctuations of Xmax and Primary Particle Mass Composition in the Range of Energy 5 10^{17} - 3 10^{19} ev by Yakutsk Data

S. P. Knurenko, A. A. Ivanov, V. A. Kolosov +3

The experimental distributions of $\Xmax$ obtained with the Yakutsk EAS array at fixed energies of , and eV are analysed. A recen…

astro-ph2004★ 6 cited

Muons with E_th >= 1 Gev and Mass Composition in the Energy Range 10^{18}-10^{20} ev Observed by Yakutsk Eas Array

S. P. Knurenko, V. A. Kolosov, I. T. Makarov +3

The ratio of the muon flux density to charged particle flux density at distances of 300 and 600 m from the shower axis ($\rhom(300)/\rhos(300)$ and $\rhom(600)/\rhos(600)$) is meas…

astro-ph2004★ 3 cited

Influence of Primary Cosmic Radiation Mass Composition on the Estimation of Eas Energy

S. P. Knurenko, A. A. Ivanov, V. A. Kolosov +3

At the Yakutsk EAS array E_em is determined by using measurements of EAS Cherenkov light flux and charged particle flux. It is known from calculations that these characteristics de…

astro-ph2004★ 73 cited

The spectrum features of UHECRs below and surrounding GZK

V. P. Egorova, A. V. Glushkov, A. A. Ivanov +10

The energy spectrum of UHECRs is discussed on the basis of the Yakutsk array database analysis. In the region E=0.1 to 30 EeV the showers are detected under trigger-500, while at e…