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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 |