КФУ. Карточка публикации. Schwarzschild black hole as particle accelerator of spinning particles

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SCHWARZSCHILD BLACK HOLE AS PARTICLE ACCELERATOR OF SPINNING PARTICLES

Форма представления

Статьи в зарубежных журналах и сборниках

Год публикации

2016

Язык

русский

Авторы, сотрудники КФУ

Заславский Олег Борисович, автор

Библиографическое описание на языке оригинала

O. B. Zaslavskii, Schwarzschild black hole as particle accelerator of spinning particles, Europhys. Lett. 114 (2016) 30003.

Аннотация

It is shown that in the Schwarzschild background there exists a direct counterpart of the Ba˜nados-Silk-West effect for spinning particles. This means that if two particles collide near the black-hole horizon, their energy in the centre-of-mass frame can grow unbounded. In doing so, the crucial role is played by the so-called near-critical trajectories when the particle parameters are almost fine-tuned. A direct scenario of the collision under discussion is possible with restriction on the energy-to-mass ratio. However, if one takes into account multiple scattering, this becomes possible for E>m as well.

Ключевые слова

Spin, BSW effect

Название журнала

EPL

URL

http://iopscience.iop.org/article/10.1209/0295-5075/114/30003/pdf

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https://repository.kpfu.ru/?p_id=166664

Полная запись метаданных

Поле DC	Значение	Язык
dc.contributor.author	Заславский Олег Борисович	ru_RU
dc.date.accessioned	2016-01-01T00:00:00Z	ru_RU
dc.date.available	2016-01-01T00:00:00Z	ru_RU
dc.date.issued	2016	ru_RU
dc.identifier.citation	O. B. Zaslavskii, Schwarzschild black hole as particle accelerator of spinning particles, Europhys. Lett. 114 (2016) 30003.	ru_RU
dc.identifier.uri	https://repository.kpfu.ru/?p_id=166664	ru_RU
dc.description.abstract	EPL	ru_RU
dc.description.abstract	It is shown that in the Schwarzschild background there exists a direct counterpart of the Ba˜nados-Silk-West effect for spinning particles. This means that if two particles collide near the black-hole horizon, their energy in the centre-of-mass frame can grow unbounded. In doing so, the crucial role is played by the so-called near-critical trajectories when the particle parameters are almost fine-tuned. A direct scenario of the collision under discussion is possible with restriction on the energy-to-mass ratio. However, if one takes into account multiple scattering, this becomes possible for E>m as well.	ru_RU
dc.language.iso	ru	ru_RU
dc.subject	Spin	ru_RU
dc.subject	BSW effect	ru_RU
dc.title	Schwarzschild black hole as particle accelerator of spinning particles	ru_RU
dc.type	Статьи в зарубежных журналах и сборниках	ru_RU