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Космология, первичные черные дыры и сверхмассивные частицы

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Анализ астрофизических ограничений на спектр первичных черных дыр (ПЧЛ) позволяет получить косвенную информацию о физических условиях в очень ранней Вселенной. Указанные ограничения сопоставляются с вероятностью образования ПЧЛ на ранних пылевидных стадиях, предсказываемых на основе современных моделей квантовой теории поля. В результате такого сопоставления получены ограничения на параметры различных моделей в зависимости от параметров спектра начальных мелкомасштабных неоднородностей. Ил. 9, библиогр. ссылок 127 (178 назв.).

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English fulltext is available at DOI: 10.1070/PU1985v028n03ABEH003858
PACS: 04.70.Dy, 98.80.Cq, 14.80.Hv, 11.30.Ly, 11.10.−z (все)
DOI: 10.3367/UFNr.0145.198503a.0369
URL: https://ufn.ru/ru/articles/1985/3/a/
Цитата: Полнарев А Г, Хлопов М Ю "Космология, первичные черные дыры и сверхмассивные частицы" УФН 145 369–401 (1985)
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English citation: Polnarev A G, Khlopov M Yu “Cosmology, primordial black holes, and supermassive particles” Sov. Phys. Usp. 28 213–232 (1985); DOI: 10.1070/PU1985v028n03ABEH003858

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