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Колебательный режим приближения к особой точке в релятивистской космологии

СОДЕРЖАНИЕ
1. Введение
2. Обобщенное решение Казнера
3. Колебательный режим приближения к особой точке
4. Эволюция модели под влиянием двух возмущений
5. Эволюция модели в асимптотической области сколь угодно малых времен
6. Статистический анализ эволюции модели при приближении к особой точке
7. Построение общего решения для длинной эры с малыми колебаниями
8. Заключительные замечания
Приложения
A. Некоторые сведения из теории непрерывных дробей
Б. Уточнение расчетов к разделу 4
B. Однородные пространства
Г. Однородные пространства типов VII и IX
Цитированная литература

Текст pdf (2,5 Мб)
English fulltext is available at DOI: 10.1070/PU1971v013n06ABEH004279
PACS: 98.80.Jk, 04.20.Jb, 95.30.Sf (все)
DOI: 10.3367/UFNr.0102.197011d.0463
URL: https://ufn.ru/ru/articles/1970/11/d/
Цитата: Белинский В А, Лифшиц Е М, Халатников И М "Колебательный режим приближения к особой точке в релятивистской космологии" УФН 102 463–500 (1970)
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English citation: Belinskii V A, Lifshitz E M, Khalatnikov I M “Oscillatory approach to the singular point in relativistic cosmologySov. Phys. Usp. 13 745–765 (1971); DOI: 10.1070/PU1971v013n06ABEH004279

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