69 citations · 84 across the 8 of their papers we have counts for
8 papers
Effect of paramagnetic impurities on superconductivity in polyhydrides: -wave order parameter in Nd-doped LaH
Dmitrii V. Semenok, Ivan A. Troyan, Andrey V. Sadakov +19
Polyhydrides are a novel class of superconducting materials with extremely high critical parameters, which is very promising for applications. On the other hand, complete experimen…
Analog of the Intertype Superconductivity in Nanostructured Materials
D. M. Gokhfeld, S. I. Popkov, A. A. Bykov
Magnetization hysteresis loops of tin samples with an inverted opal structure are presented. The sample formed by tin particles with the size of 70 and 128 nm is found to be a type…
Magnetoresistance Relaxation in (La0.5Eu0.5)0.7Pb0.3MnO3 Single Crystals under the Action of a Pulse Magnetic Field
A. A. Bykov, S. I. Popkov, K. A. Shaykhutdinov +1
Magnetoresistance of substituted lanthanum manganite (La0.5Eu0.5)0.7Pb0.3MnO3 in the pulse magnetic field H = 25 T was measured at different temperatures. Magnetoresistance relaxat…
MSW Solutions to the Solar Neutrino Problem in Presence of Noisy Matter Density Fluctuations
A. A. Bykov, M. C. Gonzalez-Garcia, C. Peña-Garay +2
We study the effect of random matter density fluctuations in the sun on resonant neutrino conversion in matter by solving numerically the evolution equation for the neutrino system…
Resonant Spin-Flavor Precession Solution to the Solar Neutrino Problem and electron antineutrinos from the Sun
A. A. Bykov, V. Yu. Popov, T. I. Rashba +1
We have found allowed squared mass difference, magnetic field, mixing angle - regions for the Resonant Spin-Flavor Precession Solution to the Solar Neutrino Problem fitted with the…
Neutrino Spin-Flavor Conversions and Electron Antineutrino emission from the Sun with Random Magnetic Field
V. B. Semikoz, A. A. Bykov, V. Yu. Popov +2
The magnetic field in the solar convective zone has a random small-scale component with the r.m.s. value substancially exceeding the strength of a regular large-scale field. For tw…