Магнито-вращательная эволюция и популяционный синтез одиночных нейтронных звезд
Диссертация
Исследованы особенности магнито-вращательной эволюции старых одиночных нейтронных звезд и получены следующие результаты. а) Рассчитаны модели эволюции одиночных нейтронных звезд с затуханием магнитного поля на большом масштабе времени для разных моделей затухания. Для разных моделей затухания выделены диапазоны параметров, при которых нейтронные звезды выходят на стадию аккреции из межзвездной… Читать ещё >
Содержание
- 1. Обзор
- 1. 1. Нейтронные звезды. Основные свойства
- 1. 1. 1. Основные тииы молодых одиночных нейтронных звезд
- 1. 2. Эволюция нейтронных звезд
- 1. 2. 1. Магнито-вращательная эволюция
- 1. 2. 2. Затухание магнитного поля
- 1. 2. 3. Тепловая эволюция
- 1. 3. Популяционный синтез
- 1. 1. Нейтронные звезды. Основные свойства
- 2. Магнито-вращательная эволюция нейтронных звезд
- 2. 1. Эволюция одиночной нейтронной звезды с затуханием магнитного поля
- 2. 1. 1. Экспоненциальное затухание ноля
- 2. 1. 2. Затухание поля по степенному закону
- 2. 2. Стохастическое поведение одиночных аккрецирующих нейтронных звезд
- 2. 2. 1. Магнито-вращательная эволюция и одиночные ак-креторы
- 2. 2. 2. Модель
- 2. 2. 3. Расчеты и результаты
- 2. 2. 4. Обсуждение и
- 2. 1. Эволюция одиночной нейтронной звезды с затуханием магнитного поля
- 2. 3. Режим трансзвукового пропеллера
- 2. 3. 1. Некоторые особенности стадии пропеллера
- 2. 3. 2. Почему должен существовать промежуточный режим?
- 2. 3. 3. Трансзвуковой пропеллер
- 2. 3. 4. Обсуждение
- 2. 3. 5. Выводы
- 2. 4. Эволюция периодов нейтронных звезд и их эволюционный статус на стадии, предшествующей классическим маломассивным рентгеновским двойным
- 2. 4. 1. Модель
- 2. 4. 2. Результаты
- 2. 4. 3. Обсуждение и подведение итогов
- 2. 5. Роль двойных систем в вопросе о корреляции между осью вращения и вектором пространственной скорости одиночных нейтронных звезд
- 2. 5. 1. Популяционная модель
- 2. 5. 2. Результаты расчетов
- 2. 5. 3. Обсуждение
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