Effective temperature of vacuum and particles on the horizons

An approach has been proposed in which the evolution of horizons is determined by their effective temperature. Effective horizon lifetimes are evaluated for two spherically symmetric metrics. It has been obtained that the charge in the Reissner–Nordstro¨ m metric is lost much faster than its mass, and that Kottler’s metric vacuum in the early Universe may decay faster than Schwarzschild’s horizon evaporates. The results obtained may be of importance for black hole physics and cosmology. © 2017, Pleiades Publishing, Ltd.

Редакторы
-
Издательство
-
Номер выпуска
1
Язык
Английский
Страницы
80-83
Статус
Опубликовано
Подразделение
-
Номер
-
Том
23
Год
2017
Организации
  • 1 Institute of Gravitation and Cosmology, Peoples’ Friendship University of Russia, ul. Miklukho-Maklaya 6, Moscow, 117198, Russian Federation
Ключевые слова
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Дата создания
19.10.2018
Дата изменения
19.10.2018
Постоянная ссылка
https://repository.rudn.ru/ru/records/article/record/5744/