Диссертация (1149660), страница 14
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В выполненныхздесь конкретных численных экспериментах для случаев с максимально воз-87можными колебаниями , величины никогда не достигают критического значения = + 0.5 (2.31). Поскольку орбитальный момент остается меньшим (2.31), его величина выпадает из теории в силу слабой зависимости от как критического значения напряженности поля (2.44), так и соответствующего коэффициента диффузии в уравнениях типа Фоккера–Планка [60, 63] вдиапазоне < .88Список литературы1. Nielsen M. A., Chuang I.
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