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 |
|