1999/04/30 by A. V. Kuznetsov, А. В. Кузнецов, Н. В. Михеев +1 · 14 citations
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Atomic physics #Electron #Magnetic field #Neutrino #Neutrino Physics Research #Nuclear physics #Physics #Plasma #Quantum mechanics #Quantum, superfluid, helium dynamics #astro-ph #hep-ph
paper · pdf · doi:10.1142/s0217732399002649
published in Modern Physics Letters A 14(36), 2531-2536 (World Scientific) · 8 pages, LATEX, no figures, minor improvements, conclusions not changed
arxiv created 1999/11/23 · openalex publication_date 1999/11/30 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The total set of the neutrino–electron processes in the presence of both components of an active medium, hot dense plasma and strong magnetic field, is investigated for the first time. The contribution of the processes νe - →νe - , νe + →νe + , ν→νe - e + , νe - e + →ν is shown to dominate and not to depend on the chemical potential of electron–positron gas. Relatively simple expressions for the probability and mean losses of the neutrino energy and momentum are obtained, which are suitable for a quantitative analysis.