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Kinematics of ultra-high energy particle collisions near black holes in the magnetic field

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dc.contributor.author Zaslavskii O.
dc.date.accessioned 2018-09-18T20:07:13Z
dc.date.available 2018-09-18T20:07:13Z
dc.date.issued 2015
dc.identifier.issn 0217-7323
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/136693
dc.description.abstract © 2015 World Scientific Publishing Company. There are different versions of collisions of two particles near black holes with unbound energy E<inf>cm</inf> in the center of mass frame. The so-called BSW effect arises when a slow fine-tuned "critical" particle hits a rapid "usual" one. We discuss a scenario of collision in the strong magnetic field for which explanation turns out to be different. Both particles are rapid but the nonzero angle between their velocities (which are both close to c, the speed of light) results in a relative velocity close to c and, hence, big E<inf>cm</inf>.
dc.relation.ispartofseries Modern Physics Letters A
dc.subject BSW effect
dc.subject magnetic field
dc.title Kinematics of ultra-high energy particle collisions near black holes in the magnetic field
dc.type Article
dc.relation.ispartofseries-issue 6
dc.relation.ispartofseries-volume 30
dc.collection Публикации сотрудников КФУ
dc.source.id SCOPUS02177323-2015-30-6-SID84928472873


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  • Публикации сотрудников КФУ Scopus [24551]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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