339 citations · 623 across the 20 of their papers we have counts for
20 papers
HERO (High Energy Ray Observatory) optimization and current status
Alexander Kurganov, Dmitry Karmanov, Alexander Panov +3
The High-Energy Ray Observatory (HERO) is a space experiment based on a heavy ionization calorimeter for direct study of cosmic rays. The effective geometrical factor of the appara…
Search for Astrophysical Nanosecond Optical Transients with TAIGA-HiSCORE Array
A. D. Panov, I. I. Astapov, A. K. Awad +81
A wide-angle Cerenkov array TAIGA-HiSCORE (FOV 0.6 sr), was originally created as a part of TAIGA installation for high-energy gamma-ray astronomy and cosmic ray physics. Arr…
A possibility of interpretation of the cosmic ray kneenear 10 TV as a contribution of a single close source
D. Karmanov, I. Kovalev, I. Kudryashov +5
This article presents a description of a cosmic rays diffusive propagationmodel of a close point-like flash lamp like source and an approximation ofexperimentally observed spectral…
Dynamical generalizations of the Drake equation: the linear and non-linear theories
A. D. Panov
The Drake equation pertains to the essentially equilibrium situation in a population of communicative civilizations (CCs) of the Galaxy, but it does not describe dynamical processe…
A new universal cosmic-ray knee near the magnetic rigidity 10 TV with the NUCLEON space observatory
E. Atkin, V. Bulatov, V. Dorokhov +18
Data from the NUCLEON space observatory give a strong indication of the existence of a new universal cosmic ray "knee", which is observed in all groups of nuclei, including heavy n…
Energy Spectra of Abundant Cosmic-ray Nuclei in Sources, According to the ATIC Experiment
A. D. Panov, N. V. Sokolskaya, V. I. Zatsepin
One of the main results of the ATIC (Advanced Thin Ionization Calorimeter) experiment is a collection of energy spectra of abundant cosmic-ray nuclei: protons, He, C, O, Ne, Mg, Si…
First results of the cosmic ray NUCLEON experiment
E. Atkin, V. Bulatov, V. Dorokhov +19
The NUCLEON experiment was designed to study the chemical composition and energy spectra of galactic cosmic ray nuclei from protons to zinc at energies of --\…
Upturn observed in heavy nuclei to iron ratios by the ATIC-2 experiment
A. D. Panov, N. V. Sokolskaya, V. I. Zatsepin +15
The ratios of fluxes of heavy nuclei from sulfur (Z=16) to chromium (Z=24) to the flux of iron were measured by the ATIC-2 experiment. The ratios are decreasing functions of energy…
To the interpretation of the upturn observed by ATIC in heavy nuclei to iron ratios
A. D. Panov, N. V. Sokolskaya, V. I. Zatsepin
It is argued that the upturn observed in heavy nuclei to iron ratios as measured in the ATIC experiment could be understood within the model of closed galaxy with embedded local re…
A United Model for the cosmic ray energy spectra and anisotropy in the energy range 100 - 100 000 GeV
V. I. Zatsepin, A. D. Panov, N. V. Sokolskaya
We propose a model where a supernova explodes in some vicinity of our solar system (some tens of parsecs) in the recent past (some tens of thousands years) with the energy release…
Possible structure in the cosmic ray electron spectrum measured by the ATIC-2 and ATIC-4 experiments
A. D. Panov, V. I. Zatsepin, N. V. Sokolskaya +15
A strong excess in a form of a wide peak in the energy range of 300-800 GeV was discovered in the first measurements of the electron spectrum in the energy range from 20 GeV to 3 T…
Energy Spectra of Abundant Nuclei of Primary Cosmic Rays from the Data of ATIC-2 Experiment: Final Results
A. D. Panov, J. H. Adams, H. S. Ahn +17
The final results of processing the data from the balloon-born experiment ATIC-2 (Antarctica, 2002-2003) for the energy spectra of protons and He, C, O, Ne, Mg, Si, and Fe nuclei,…
Energy dependence of Ti/Fe ratio in the Galactic cosmic rays measured by the ATIC-2 experiment
V. I. Zatsepin, A. D. Panov, N. V. Sokolskaya +15
Titanium is a rare, secondary nucleus among Galactic cosmic rays. Using the Silicon matrix in the ATIC experiment, Titanium has been separated. The energy dependence of the Ti to F…
Relative abundances of cosmic ray nuclei B-C-N-O in the energy region from 10 GeV/n to 300 GeV/n. Results from ATIC-2 (the science flight of ATIC)
A. D. Panov, N. V. Sokolskaya, J. H. Adams +19
The ATIC balloon-borne experiment measures the energy spectra of elements from H to Fe in primary cosmic rays from about 100 GeV to 100 TeV. ATIC is comprised of a fully active bis…
The results of ATIC-2 experiment for elemental spectra of cosmic rays
A. D. Panov, J. H. Adams, H. S. Ahn +19
The results of ATIC-2 baloon experiment (2002-2003) for energy spectra of protons, He, C, O, Ne, Mg, Si, Fe, some groups of nuclei, and all-particle spectrum in primary cosmic rays…
Inverse Quantum Zeno Effect in Quantum Oscillations
Alexander D. Panov
It is shown that inverse quantum Zeno effect (IZE) may exist in a three-level system with Rabi oscillations between discrete atomic states. The experiment to observe IZE in such a…
Computer Model of Quantum Zeno Effect in Spontaneous Decay with Distant Detector
Alexander D. Panov
A numerical model of spontaneous decay continuously monitored by a distant detector of emitted particles is constructed. It is shown that there is no quantum Zeno effect in such qu…
Quantum Zeno-like effect and spectra of particles in cascade transition
Alexander D. Panov
Shrödinger equation for two-step spontaneous cascade transition in a three-level quantum system is solved by means of Markovian approximation for non-Markovian integro-differential…
General equation for Zeno-like effects in spontaneous exponential decay
Alexander D. Panov
It was shown that different mechanisms of perturbation of spontaneous decay constant: inelastic interaction of emitted particles with particle detector, decay onto an unstable leve…
Zeno effect preventing Rabi transitions onto an unstable energy level
J. Audretsch, M. B. Mensky, A. D. Panov
We consider a driven 2-level system with one level showing spontaneous decay to an otherwise uncoupled third level. Rabi transitions to the unstable level are strongly damped. This…