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High energy particle collisions near black holes

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dc.contributor Казанский (Приволжский) федеральный университет
dc.contributor.author Заславский Олег Борисович ru_RU
dc.date.accessioned 2016-12-12T07:20:10Z
dc.date.available 2016-12-12T07:20:10Z
dc.date.issued 2016
dc.identifier.uri http://dspace.kpfu.ru/xmlui/handle/net/108454
dc.description.abstract If two geodesic particles collide near a rotating black hole, their energy in the centre of mass frame Ec.m. can become unbound under certain conditions (the so-called BSW effect). The special role is played here by so-called critical geodesics when one of particles has fine-tuned energy and angular momentum. The nature of geodesics reveals itself also in fate of the debris after collisions. One of particles moving to a remote observer is necessarily near-critical. We discuss, when such a collision can give rise not only unboud Ec.m. but also unbound Killing energy E (so-called super-Penrose process). en_US
dc.relation.ispartofseries Международная школа "Математическое моделирование фундаментальных объектов и явлений в системах компьютерной математики - KAZCAS-2016". Международный научный семинар "Нелинейные модели в механике, статистике, теории поля и космологии - GRACOS-16 ru_RU
dc.subject particle collision en_US
dc.subject centre of mass en_US
dc.subject Penrose process en_US
dc.title High energy particle collisions near black holes en_US
dc.type article
dc.identifier.udk 530.12
dc.description.pages 66-72


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