On the limiting energy of the collision of elementary particles close to horizon of the rotating black hole

dc.contributor.author	Grib A.A.
dc.contributor.author	Pavlov Y.V.
dc.date.accessioned	2021-02-25T20:34:33Z
dc.date.available	2021-02-25T20:34:33Z
dc.date.issued	2020
dc.identifier.issn	0217-7323
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/161797
dc.description.abstract	© 2020 World Scientific Publishing Company. Arguments are given for the conclusion that the energy of collision of two ultrarelativistic elementary particles due to gravitational radiation cannot exceed the Planck value. Comparison of the gravitational and electromagnetic radiation for charged particles close to the horizon of Kerr black hole is made. If for trans-Planckian energy the black hole can arise it is shown that the energy growth used in scattering for interaction of particles is still limited.
dc.relation.ispartofseries	Modern Physics Letters A
dc.subject	black hole
dc.subject	gravitational radiation
dc.subject	Ultra-high energy collision
dc.title	On the limiting energy of the collision of elementary particles close to horizon of the rotating black hole
dc.type	Article
dc.relation.ispartofseries-issue	31
dc.relation.ispartofseries-volume	35
dc.collection	Публикации сотрудников КФУ
dc.source.id	SCOPUS02177323-2020-35-31-SID85093826052

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Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.