Application of inverse Z-pinch for study of the pd reaction at keV energy range

V. M. Bystritsky, Vit M. Bystritskii, G. N. Dudkin, V. V. Gerasimov, A. R. Krylov, G. A. Mesyats, B. A. Nechaev, V. M. Padalko, S. S. Parzhitsky, F. M. Pen'kov, N. A. Ratakhin, V. A. Stolupin, J. Wozniak

Результат исследований: Материалы для журналаСтатья

10 Цитирования (Scopus)

Выдержка

Formation and dynamics of the hydrogen liner, and nuclear reaction (pd→3He+γ (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 Hα-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.

Язык оригиналаАнглийский
Страницы (с-по)864-875
Число страниц12
ЖурналNuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Том565
Номер выпуска2
DOI
СостояниеОпубликовано - 15 сен 2006

Отпечаток

linings
Protons
protons
Plasmas
astrophysics
energy distribution
plasma radiation
Astrophysics
collisions
Nuclear reactions
energy
nuclear reactions
deuterons
Physics
Radiation
Hydrogen
physics
nuclei
cross sections
hydrogen

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Instrumentation

Цитировать

Application of inverse Z-pinch for study of the pd reaction at keV energy range. / Bystritsky, V. M.; Bystritskii, Vit M.; Dudkin, G. N.; Gerasimov, V. V.; Krylov, A. R.; Mesyats, G. A.; Nechaev, B. A.; Padalko, V. M.; Parzhitsky, S. S.; Pen'kov, F. M.; Ratakhin, N. A.; Stolupin, V. A.; Wozniak, J.

В: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Том 565, № 2, 15.09.2006, стр. 864-875.

Результат исследований: Материалы для журналаСтатья

Bystritsky, V. M. ; Bystritskii, Vit M. ; Dudkin, G. N. ; Gerasimov, V. V. ; Krylov, A. R. ; Mesyats, G. A. ; Nechaev, B. A. ; Padalko, V. M. ; Parzhitsky, S. S. ; Pen'kov, F. M. ; Ratakhin, N. A. ; Stolupin, V. A. ; Wozniak, J. / Application of inverse Z-pinch for study of the pd reaction at keV energy range. В: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 2006 ; Том 565, № 2. стр. 864-875.
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abstract = "Formation and dynamics of the hydrogen liner, and nuclear reaction (pd→3He+γ (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 Hα-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.",
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AU - Bystritsky, V. M.

AU - Bystritskii, Vit M.

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AU - Gerasimov, V. V.

AU - Krylov, A. R.

AU - Mesyats, G. A.

AU - Nechaev, B. A.

AU - Padalko, V. M.

AU - Parzhitsky, S. S.

AU - Pen'kov, F. M.

AU - Ratakhin, N. A.

AU - Stolupin, V. A.

AU - Wozniak, J.

PY - 2006/9/15

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N2 - Formation and dynamics of the hydrogen liner, and nuclear reaction (pd→3He+γ (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 Hα-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.

AB - Formation and dynamics of the hydrogen liner, and nuclear reaction (pd→3He+γ (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 Hα-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.

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