000 | 03756nlm0a2200505 4500 | ||
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001 | 654982 | ||
005 | 20231030041323.0 | ||
035 | _a(RuTPU)RU\TPU\network\20756 | ||
035 | _aRU\TPU\network\10227 | ||
090 | _a654982 | ||
100 | _a20170607a2013 k y0engy50 ba | ||
101 | 0 |
_aeng _deng |
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102 | _aNL | ||
105 | _ay z 100zy | ||
135 | _adrcn ---uucaa | ||
181 | 0 | _ai | |
182 | 0 | _ab | |
200 | 1 |
_aSlowing-down of relativistic heavy ions and its influence on angular distributions of Vavilov–Cherenkov radiation _fE. I. Fiks [et al.] |
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203 |
_aText _celectronic |
||
300 | _aTitle screen | ||
320 | _a[References: p. 54 (14 tit.)] | ||
330 | _aWe performed calculations of Vavilov-Cherenkov radiation (VChR) angular distributions from relativistic heavy ions (RHI) taking account of their slowing-down in a radiator. The results of calculations show that the slowing-down of RHI in radiator leads to specific broadening of VChR ring thus forming specific VChR angular distribution which is different compared to well-known Tamm-Frank distribution. The key parameters which change drastically the VChR angular distribution from RHI are: energy, charge and mass of an ion; emission wave length and corresponding refractive index; stopping power and radiator thickness. The theory developed has been applied to the analysis of the earlier experiments (1996-2001) devoted to studies of the VChR angular distribution from Au RHI beam with energies ∼0.9 GeV/u at SIS-18 heavy ion accelerator (GSI, Darmstadt, Germany). | ||
333 | _aРежим доступа: по договору с организацией-держателем ресурса | ||
461 |
_tNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms _oScientific Journal _d1984- |
||
463 |
_tVol. 314 : Swift Heavy Ions in Matter (SHIM 2012) _oproceedings of the Eighth International Symposium, October 24-27, 2012, Kyoto, Japan _v[P. 51-54] _d2013 |
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610 | 1 | _aэлектронный ресурс | |
610 | 1 | _aтруды учёных ТПУ | |
610 | 1 | _aчеренковское излучение | |
610 | 1 | _aэнергия | |
610 | 1 | _aпотери | |
610 | 1 | _aрелятивистские тяжелые ионы | |
610 | 1 | _acherenkov radiation | |
610 | 1 | _aenergy loss | |
610 | 1 | _arelativistic | |
701 | 1 |
_aFiks _bE. I. _cphysicist _cengineer-researcher of Tomsk Polytechnic University, candidate of physico-mathematical Sciences _f1988- _gElena Ivanovna _2stltpush _3(RuTPU)RU\TPU\pers\33634 |
|
701 | 1 |
_aPivovarov _bYu. L. _cphysicist _cprofessor of Tomsk Polytechnic University _f1953- _gYuriy Leonidovich _2stltpush _3(RuTPU)RU\TPU\pers\31522 |
|
701 | 1 |
_aBogdanov _bO. V. _cphysicist _cassociate professor of Tomsk Polytechnic University _f1981- _gOleg Viktorovich _2stltpush _3(RuTPU)RU\TPU\pers\31518 |
|
701 | 1 |
_aGeissel _bH. |
|
701 | 1 |
_aScheidenberger _bC. |
|
701 | 1 |
_aRuzicka _bJ. |
|
712 | 0 | 2 |
_aНациональный исследовательский Томский политехнический университет (ТПУ) _bФизико-технический институт (ФТИ) _bКафедра экспериментальной физики (ЭФ) _h7596 _2stltpush _3(RuTPU)RU\TPU\col\21255 |
712 | 0 | 2 |
_aНациональный исследовательский Томский политехнический университет (ТПУ) _bФизико-технический институт (ФТИ) _bКафедра высшей математики и математической физики (ВММФ) _h139 _2stltpush _3(RuTPU)RU\TPU\col\18727 |
801 | 2 |
_aRU _b63413507 _c20170613 _gRCR |
|
856 | 4 | _uhttps://doi.org/10.1016/j.nimb.2013.05.033 | |
942 | _cCF |