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dc.contributor.author | Zaslavskii O. | |
dc.date.accessioned | 2018-09-18T20:07:12Z | |
dc.date.available | 2018-09-18T20:07:12Z | |
dc.date.issued | 2014 | |
dc.identifier.issn | 0217-7323 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/136688 | |
dc.description.abstract | © 2014 World Scientific Publishing Company. We consider collision of two particles in the axially symmetric black hole metric in the magnetic field. If the value of the angular momentum |L| of one particles grows unbound (but its Killing energy remains fixed) one can achieve unbound energy in the center-of-mass frame E<inf>c.m.</inf> In the absence of the magnetic field, collision of this kind is known to happen in the ergoregion. However, if the magnetic field strength B is also large, with the ratio |L|/B being finite, large E<inf>c.m.</inf> can be achieved even far from a black hole, in the almost flat region. Such an effect also occurs in the metric of a rotating star. | |
dc.relation.ispartofseries | Modern Physics Letters A | |
dc.subject | Center-of-mass | |
dc.subject | Ergosphere | |
dc.subject | Magnetic field | |
dc.title | High-energy collision of particles in the magnetic field far from black holes | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 29 | |
dc.relation.ispartofseries-volume | 29 | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS02177323-2014-29-29-SID84929579426 |