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dc.contributor.author | Zaslavskii O. | |
dc.date.accessioned | 2018-09-19T20:29:09Z | |
dc.date.available | 2018-09-19T20:29:09Z | |
dc.date.issued | 2016 | |
dc.identifier.issn | 0295-5075 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/142945 | |
dc.description.abstract | © CopyrightEPLA, 2016.It is shown that in the Schwarzschild background there exists a direct counterpart of the Bañados-Silk-West effect for spinning particles. This means that if two particles collide near the black-hole horizon, their energy in the centre-of-mass frame can grow unbounded. In doing so, the crucial role is played by the so-called near-critical trajectories when the particle parameters are almost fine-tuned. A direct scenario of the collision under discussion is possible with restriction on the energy-to-mass ratio only. However, if one takes into account multiple scattering, this becomes possible 1for as well. | |
dc.relation.ispartofseries | EPL | |
dc.title | Schwarzschild black hole as particle accelerator of spinning particles | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 3 | |
dc.relation.ispartofseries-volume | 114 | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS02955075-2016-114-3-SID84975797040 |