Výsledky vyhledávání - "Popov, V. Yu."

Akademický článek

Simulation of a Multifractal Turbulent Electromagnetic Field in Cosmic Plasma.

Autor: Levashov, N. N.^1,2 (AUTHOR) nn.levashov@physics.msu.ru, Popov, V. Yu.^1,2,3 (AUTHOR), Malova, H. V.^3,4 (AUTHOR), Zelenyi, L. M.² (AUTHOR)

Publikováno v: Cosmic Research. Apr2023, Vol. 61 Issue 2, p113-119. 7p.

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MSW Solutions to the Solar Neutrino Problem in Presence of Noisy Matter Density Fluctuations

Autor: Bykov, A. A., Gonzalez-Garcia, M. C., Peña-Garay, C., Popov, V. Yu., Semikoz, V. B.

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 including the full effect of the random matter density fluctuations o

Externí odkaz: http://arxiv.org/abs/hep-ph/0005244

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Resonant Spin-Flavor Precession Solution to the Solar Neutrino Problem and electron antineutrinos from the Sun

Autor: Bykov, A. A., Popov, V. Yu., Rashba, T. I., Semikoz, V. B.

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 data of all acting solar neutrino experiments. The typical mass diffe

Externí odkaz: http://arxiv.org/abs/hep-ph/0002174

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Neutrino Spin-Flavor Conversions and Electron Antineutrino emission from the Sun with Random Magnetic Field

Autor: Semikoz, V. B., Bykov, A. A., Popov, V. Yu., Rez, A. I., Sokoloff, D. D.

Publikováno v: Nucl.Phys.Proc.Suppl. 81 (2000) 124-129

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 two Majorana neutrino flavors and two helicities in the presence of a ne

Externí odkaz: http://arxiv.org/abs/hep-ph/9907253

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Neutrino conversions in random magnetic fields and $\tilde{\nu}_e$ from the Sun

Autor: Bykov, A. A., Popov, V. Yu., Rez, A. I., Semikoz, V. B., Sokoloff, D. D.

Publikováno v: Phys.Rev. D59 (1999) 063001

The magnetic field in the convective zone of the Sun has a random small-scale component with the r.m.s. value substantially exceeding the strength of a regular large-scale field. For two Majorana neutrino flavors $\times$ two helicities in the presen

Externí odkaz: http://arxiv.org/abs/hep-ph/9808342

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Aperiodic Spin-Flavor Conversions and $\tilde{\nu}_e$ from the Sun with Random Magnetic Field

Autor: Semikoz, V. B., Bykov, A. A., Popov, V. Yu., Rez, A. I., Sokoloff, D. D.

The magnetic field in the solar convective zone has a random small-scale component with the r.m.s. value substantially exceeding the strength of a regular large-scale field. For two Majorana neutrino flavors $\times$ two helicities in the presence of

Externí odkaz: http://arxiv.org/abs/hep-ph/9808274

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