dc.contributor.author |
Zaslavskii O.B. |
|
dc.date.accessioned |
2021-02-25T20:34:36Z |
|
dc.date.available |
2021-02-25T20:34:36Z |
|
dc.date.issued |
2020 |
|
dc.identifier.issn |
0217-751X |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/161801 |
|
dc.description.abstract |
© 2020 World Scientific Publishing Company. If two particles collide near a rotating black hole, their energy in the centre of mass frame can become unbounded under certain conditions. In doing so, the Killing energy E of debris at infinity is, in general, remain restricted. If E is also unbounded, this is called the super-Penrose process. We elucidate when such a process is possible and give full classification of corresponding relativistic objects for rotating space-times. We also discuss the case of a pure electric super-Penrose process that is valid even in the flat space-time. The key role in consideration is played by the Wald inequalities. |
|
dc.relation.ispartofseries |
International Journal of Modern Physics A |
|
dc.subject |
acceleration of particles |
|
dc.subject |
Black hole horizon |
|
dc.subject |
centre of mass |
|
dc.subject |
extraction of energy |
|
dc.title |
Super-Penrose process |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
2-3 |
|
dc.relation.ispartofseries-volume |
35 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.source.id |
SCOPUS0217751X-2020-35-23-SID85078974559 |
|