Форма представления | Статьи в зарубежных журналах и сборниках |
Год публикации | 2016 |
Язык | русский |
|
Заславский Олег Борисович, автор
|
Библиографическое описание на языке оригинала |
O. B. Zaslavskii, Equatorial geodesics in ergoregion of dirty black holes and zero energy observers, Gen. Relat. and Gravitation 48 (2016) 132. |
Аннотация |
If two particles collide inside the ergosphere, the energy in the center of mass frame
can be made unbound provided at least one of particles has a large negative angular
momentum [A. A. Grib and Yu. V. Pavlov, Europhys. Lett. 101 (2013) 20004]. We show
that the same condition can give rise to unbounded Killing energy of debris at infinity,
i.e. super-Penrose process. Proximity of the point of collision to the black hole horizon
is not required. |
Ключевые слова |
Ergoregion, Event horizon, Negative and zero energ |
Название журнала |
General Relativity and Gravitation
|
URL |
https://link.springer.com/article/10.1007/s10714-016-2130-6 |
Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=166667 |
Полная запись метаданных |
Поле DC |
Значение |
Язык |
dc.contributor.author |
Заславский Олег Борисович |
ru_RU |
dc.date.accessioned |
2016-01-01T00:00:00Z |
ru_RU |
dc.date.available |
2016-01-01T00:00:00Z |
ru_RU |
dc.date.issued |
2016 |
ru_RU |
dc.identifier.citation |
O. B. Zaslavskii, Equatorial geodesics in ergoregion of dirty black holes and zero energy observers, Gen. Relat. and Gravitation 48 (2016) 132. |
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/?p_id=166667 |
ru_RU |
dc.description.abstract |
General Relativity and Gravitation |
ru_RU |
dc.description.abstract |
If two particles collide inside the ergosphere, the energy in the center of mass frame
can be made unbound provided at least one of particles has a large negative angular
momentum [A. A. Grib and Yu. V. Pavlov, Europhys. Lett. 101 (2013) 20004]. We show
that the same condition can give rise to unbounded Killing energy of debris at infinity,
i.e. super-Penrose process. Proximity of the point of collision to the black hole horizon
is not required. |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
Ergoregion |
ru_RU |
dc.subject |
Event horizon |
ru_RU |
dc.subject |
Negative and zero energ |
ru_RU |
dc.title |
Equatorial geodesics in ergoregion of dirty black holes and zero energy observers |
ru_RU |
dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|