Influence of slowing down in the radiator on the Cherenkov radiation angular distributions from relativistic heavy ions at FAIR, SPS and LHC energies; Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms; Vol. 309 : Channeling 2012: Charged & Neutral Particles Channeling Phenomena

Bibliographic Details
Parent link:	Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms: Scientific Journal.— , 1984- Vol. 309 : Channeling 2012: Charged & Neutral Particles Channeling Phenomena.— 2013.— [P. 146–150]
Corporate Authors:	Национальный исследовательский Томский политехнический университет (ТПУ) Физико-технический институт (ФТИ) Кафедра экспериментальной физики (ЭФ), Национальный исследовательский Томский политехнический университет (ТПУ) Физико-технический институт (ФТИ) Кафедра высшей математики и математической физики (ВММФ)
Other Authors:	Fiks E. I. Elena Ivanovna, Pivovarov Yu. L. Yuriy Leonidovich, Bogdanov O. V. Oleg Viktorovich, Geissel H., Scheidenberger C.
Summary:	Title screen The calculations of Cherenkov radiation (ChR) angular distributions from relativistic heavy ions (RHI) at very high energies (from 30 GeV/u up to 3000 GeV/u) taking into account their slowing-down (ionization energy loss) in a radiator are performed for the first time. The slowing-down of RHI in an optically transparent solid radiator can drastically change the ChR angular distributions at RHI energies of order of 1 GeV/u. The results of calculation show that at higher RHI energies (>30 GeV/u) (FAIR, SPS and LHC), the ChR angular distribution (at the reasonable radiator thickness) is very close to the Tamm–Frank distribution and practically does not depend on the RHI slowing-down in a radiator, if only ionization energy loss is taken into account. Режим доступа: по договору с организацией-держателем ресурса
Language:	English
Published:	2013
Subjects:	электронный ресурс труды учёных ТПУ черенковское излучение энергия ионизации потери релятивистские тяжелые ионы cherenkov radiation slowing down ionization energy loss relativistic heavy ions
Online Access:	https://doi.org/10.1016/j.nimb.2013.01.064
Format:	Electronic Book Chapter
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=654983

Description
Summary:	Title screen The calculations of Cherenkov radiation (ChR) angular distributions from relativistic heavy ions (RHI) at very high energies (from 30 GeV/u up to 3000 GeV/u) taking into account their slowing-down (ionization energy loss) in a radiator are performed for the first time. The slowing-down of RHI in an optically transparent solid radiator can drastically change the ChR angular distributions at RHI energies of order of 1 GeV/u. The results of calculation show that at higher RHI energies (>30 GeV/u) (FAIR, SPS and LHC), the ChR angular distribution (at the reasonable radiator thickness) is very close to the Tamm–Frank distribution and practically does not depend on the RHI slowing-down in a radiator, if only ionization energy loss is taken into account. Режим доступа: по договору с организацией-держателем ресурса
DOI:	10.1016/j.nimb.2013.01.064

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