The astrophysical S-factor for dd-reactions at ke V-energy range

V. Bystritskii, V. Bystritsky, S. Chaikovsky, M. Filipowicz, V. Grebenyuk, E. Gula, V. Makhrin, G. Mesyats, S. Parzhitski, F. Pen'Kov, N. Ratakhin, V. Sinebryukhov, S. Sorokin, V. Stolupin, E. Volkov, J. Woźniak

Результат исследований: Материалы для журналаСтатья

9 Цитирования (Scopus)

Аннотация

The experimental results of measurements of the astrophysical S-factor for dd-reaction at keV-energy range collision energies using liner plasma technique are presented. The experiments were carried out at the high current generator of the Institute of High-Current Electronics in Tomsk, Russia. The measured values of the S-factors for the deuteron collision energies 1.80, 2.06 and 227 keV are Sdd = (114 ± 68), (64 ± 30), (53 ± 16) b · keV, respectively. The corresponding cross sections for dd-reactions, described as a product of the barrier factor and measured astrophysical S-factor, are σdd n(Ecol = 1.80 keV) = (4.3 ± 2.6) · 10-33 cm2; σdd n(Ecol = 2.06 keV) = (9.8 ± 4.6) · 10-33 cm2; σdd n(Ecol = 2.27 keV) = (2.1 ± 0.6) · 10-32 cm2.

Язык оригиналаАнглийский
Страницы (с-по)42-46
Число страниц5
ЖурналKerntechnik
Том66
Номер выпуска1-2
СостояниеОпубликовано - фев 2001
Опубликовано для внешнего пользованияДа

ASJC Scopus subject areas

  • Nuclear Energy and Engineering

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  • Цитировать

    Bystritskii, V., Bystritsky, V., Chaikovsky, S., Filipowicz, M., Grebenyuk, V., Gula, E., Makhrin, V., Mesyats, G., Parzhitski, S., Pen'Kov, F., Ratakhin, N., Sinebryukhov, V., Sorokin, S., Stolupin, V., Volkov, E., & Woźniak, J. (2001). The astrophysical S-factor for dd-reactions at ke V-energy range. Kerntechnik, 66(1-2), 42-46.