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 energies above 30 EeV the whole acceptance area for trigger-1000 is used in order to utilize all the data available in the region of GZK cutoff
The Yakutsk array observes the Cherenkov light emitted by UHECR in atmosphere. Recently, an autonomo...
The paper presents results on the longitudinal development of air showers of ultra-high energies obt...
Ultra-high energy cosmic ray (UHECR) protons produced by uniformly distributed astrophysical sources...
In this work the energy spectrum of cosmic rays based on Yakutsk EAS array data is presented. After ...
We developed a numerical simulation of the propagation of UHECR in the Cosmic Microwave Background (...
The paper describes methods used for the detection of cosmic rays with energies above 10^18 eV (UHEC...
Abstract: The GZK effect, i.e. the interaction of ultra-high-energy cosmic ray (UHECR) protons and n...
14 pages, 8 figuresWe discuss the GZK horizon of protons and present a method to constrain the injec...
The experimental data on the cosmic ray energy spectrum obtained from the Small Cherenkov Array in Y...
The experimental data on the cosmic ray energy spectrum obtained from the Small Cherenkov Array in Y...
Relic neutrino nu_r light masses clustering in Galactic and Local Hot Dark Halos act as a beam dump ...
The Telescope Array (TA) collaboration has measured the energy spectrum of ultra-high energy cosmic ...
The Telescope Array (TA) collaboration has measured the energy spectrum of ultra-high energy cosmic ...
The observed energy spectrum of ultra high energy cosmic rays (UHECR) is distorted by errors in the ...
The paper presents results on the longitudinal development of air showers of ultra-high energies obt...
The Yakutsk array observes the Cherenkov light emitted by UHECR in atmosphere. Recently, an autonomo...
The paper presents results on the longitudinal development of air showers of ultra-high energies obt...
Ultra-high energy cosmic ray (UHECR) protons produced by uniformly distributed astrophysical sources...
In this work the energy spectrum of cosmic rays based on Yakutsk EAS array data is presented. After ...
We developed a numerical simulation of the propagation of UHECR in the Cosmic Microwave Background (...
The paper describes methods used for the detection of cosmic rays with energies above 10^18 eV (UHEC...
Abstract: The GZK effect, i.e. the interaction of ultra-high-energy cosmic ray (UHECR) protons and n...
14 pages, 8 figuresWe discuss the GZK horizon of protons and present a method to constrain the injec...
The experimental data on the cosmic ray energy spectrum obtained from the Small Cherenkov Array in Y...
The experimental data on the cosmic ray energy spectrum obtained from the Small Cherenkov Array in Y...
Relic neutrino nu_r light masses clustering in Galactic and Local Hot Dark Halos act as a beam dump ...
The Telescope Array (TA) collaboration has measured the energy spectrum of ultra-high energy cosmic ...
The Telescope Array (TA) collaboration has measured the energy spectrum of ultra-high energy cosmic ...
The observed energy spectrum of ultra high energy cosmic rays (UHECR) is distorted by errors in the ...
The paper presents results on the longitudinal development of air showers of ultra-high energies obt...
The Yakutsk array observes the Cherenkov light emitted by UHECR in atmosphere. Recently, an autonomo...
The paper presents results on the longitudinal development of air showers of ultra-high energies obt...
Ultra-high energy cosmic ray (UHECR) protons produced by uniformly distributed astrophysical sources...