Kazan Federal University Digital Repository

Rotation as an origin of high energy particle collisions

Show simple item record

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


Files in this item

This item appears in the following Collection(s)

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

Show simple item record

Search DSpace


Advanced Search

Browse

My Account

Statistics