| 000 | 03041nlm1a2200493 4500 | ||
|---|---|---|---|
| 001 | 653476 | ||
| 005 | 20231030041221.0 | ||
| 035 | _a(RuTPU)RU\TPU\network\18917 | ||
| 035 | _aRU\TPU\network\18915 | ||
| 090 | _a653476 | ||
| 100 | _a20170303a2006 k y0engy50 ba | ||
| 101 | 0 | _aeng | |
| 135 | _adrcn ---uucaa | ||
| 181 | 0 | _ai | |
| 182 | 0 | _ab | |
| 200 | 1 |
_aApplication of inverse Z-pinch for study of the pd reaction at keV energy range _fV. M. Bystritsky [et al.] |
|
| 203 |
_aText _celectronic |
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| 300 | _aTitle screen | ||
| 320 | _a[References: p. 875 (20 tit.)] | ||
| 330 | _aormation and dynamics of the hydrogen liner, and nuclear reaction (pd?3He+? (5.5 MeV)) in the keV collision energy range were studied using the inverse Z-pinch configuration. The fundamental properties of light nuclei reactions in keV energy range are of importance for checking the validity of the models in basic physics and astrophysics. Two experimental techniques were proposed and tested for recovering the energy distribution of the protons in the expanding plasma liner. The first technique is based on the measuring the proton flow density, and the second on the measuring the Ha-plasma radiation of the exited neutrals in the expanding plasma liner. It is shown that the combined use of these two techniques could provide relevant information on the energy distribution of the accelerated protons in the liner. This approach was used to get the estimates of the upper limits for the astrophysical S-factor and effective cross section of the pd-reaction for proton–deuteron collisions in the energy range of 2.7–16.7 keV. | ||
| 333 | _aРежим доступа: по договору с организацией-держателем ресурса | ||
| 461 |
_tNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment _d1984- |
||
| 463 |
_tVol. 565, iss. 2 _v[P. 864-875] _d2006 |
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| 610 | 1 | _aэлектронный ресурс | |
| 610 | 1 | _aтруды учёных ТПУ | |
| 610 | 1 | _aэнергия | |
| 610 | 1 | _aZ-пинч | |
| 610 | 1 | _aядерные реакции | |
| 701 | 1 |
_aBystritsky _bV. M. _gVyacheslav Mikhaylovich |
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| 701 | 1 |
_aBystritskii _bV. M. |
|
| 701 | 1 |
_aDudkinc _bG. N. |
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| 701 | 1 |
_aGerasimov _bV. V. |
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| 701 | 1 |
_aKrylova _bA. R. |
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| 701 | 1 |
_aMesyats _bG. A. _crussian physicist _cacademican, vice-president of RAS _cgraduate of Tomsk Polytechnic Institute _f1936- _gGennady Andreyevich _2stltpush _3(RuTPU)RU\TPU\pers\28088 |
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| 701 | 1 |
_aNechaev _bV. A. |
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| 701 | 1 |
_aPadalko _bV. M. |
|
| 701 | 1 |
_aParzhitsky _bS. S. |
|
| 701 | 1 |
_aPen’kova _bF. M. |
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| 701 | 1 |
_aRatakhin _bN. A. _cphysicist _cHead of the Department of Tomsk Polytechnic University, Doctor of physical and mathematical sciences _f1950- _gNikolay Aleksandrovich _2stltpush _3(RuTPU)RU\TPU\pers\36686 |
|
| 701 | 1 |
_aStolupin _bV. A. |
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| 701 | 1 |
_aWozniak _bJ. |
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| 801 | 2 |
_aRU _b63413507 _c20170403 _gRCR |
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| 856 | 4 | _uhttp://dx.doi.org/10.1016/j.nima.2006.05.262 | |
| 942 | _cCF | ||