Показать сокращенную информацию
dc.contributor.author | Pavlov Y. | |
dc.contributor.author | Zaslavskii O. | |
dc.date.accessioned | 2020-01-15T20:52:04Z | |
dc.date.available | 2020-01-15T20:52:04Z | |
dc.date.issued | 2019 | |
dc.identifier.issn | 0001-7701 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/155445 | |
dc.description.abstract | © 2019, Springer Science+Business Media, LLC, part of Springer Nature. We consider a particle moving towards a rotating black hole. We are interested in the number of its revolution n around a black hole. In our previous work (Pavlov and Zaslavskii in Gen Relativ Gravit 50:14, 2018. arXiv:1707.02860) we considered this issue in the Boyer–Lindquist type of coordinates with a subsequent procedure of subtraction. Now, we reconsider this issue using from the very beginning the frames regular on the horizon. For a nonextremal black hole, regularity of a coordinate frame leads to the finiteness of a number of revolutions around a black hole without a subtraction procedure. Meanwhile, for extremal black holes comparison of n calculated in the regular frame with some subtraction procedures used by us earlier shows that the results can be different. | |
dc.relation.ispartofseries | General Relativity and Gravitation | |
dc.subject | Black holes | |
dc.subject | Critical particles | |
dc.subject | Nonextremal and extremal horizons | |
dc.subject | Rotating frames | |
dc.subject | Rotational analogue of Eddington–Finkelstein frames | |
dc.title | Regular frames and particle’s rotation near a black hole | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 5 | |
dc.relation.ispartofseries-volume | 51 | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS00017701-2019-51-5-SID85065636296 |