Form of presentation | Articles in international journals and collections |
Year of publication | 2016 |
Язык | русский |
|
Zaslavskiy Oleg Borisovich, author
|
Bibliographic description in the original language |
O. B. Zaslavskii, Equatorial geodesics in ergoregion of dirty black holes and zero energy observers, Gen. Relat. and Gravitation 48 (2016) 132. |
Annotation |
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. |
Keywords |
Ergoregion, Event horizon, Negative and zero energ |
The name of the journal |
General Relativity and Gravitation
|
URL |
https://link.springer.com/article/10.1007/s10714-016-2130-6 |
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=166667&p_lang=2 |
Full metadata record |
Field DC |
Value |
Language |
dc.contributor.author |
Zaslavskiy Oleg Borisovich |
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/eng/?p_id=166667&p_lang=2 |
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 |
Articles in international journals and collections |
ru_RU |
|