Rotation as an origin of high energy particle collisions

dc.contributor.author	Zaslavskii O.
dc.date.accessioned	2018-09-19T20:25:15Z
dc.date.available	2018-09-19T20:25:15Z
dc.date.issued	2016
dc.identifier.issn	0217-7323
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/142890
dc.description.abstract	© 2016 World Scientific Publishing Company.We consider collision of two particles in rotating spacetimes without horizons. If the metric coefficient responsible for rotation of spacetime is big enough, the energy of collisions in the center of mass frame can be as large as one likes. This can happen in the ergoregion only. The results are model-independent and apply both to relativistic stars and wormholes.
dc.relation.ispartofseries	Modern Physics Letters A
dc.subject	acceleration of particles
dc.subject	center of mass
dc.subject	Particle collision
dc.title	Rotation as an origin of high energy particle collisions
dc.type	Article
dc.relation.ispartofseries-issue	4
dc.relation.ispartofseries-volume	31
dc.collection	Публикации сотрудников КФУ
dc.source.id	SCOPUS02177323-2016-31-4-SID84959375799

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