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

Abstract

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 S_dd = (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 σ_dd ⁿ(E_col = 1.80 keV) = (4.3 ± 2.6) · 10^-33 cm²; σ_dd ⁿ(E_col = 2.06 keV) = (9.8 ± 4.6) · 10^-33 cm²; σ_dd ⁿ(E_col = 2.27 keV) = (2.1 ± 0.6) · 10^-32 cm².

Original language	English
Pages (from-to)	42-46
Number of pages	5
Journal	Kerntechnik
Volume	66
Issue number	1-2
Publication status	Published - Feb 2001
Externally published	Yes

ASJC Scopus subject areas

Nuclear Energy and Engineering

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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.

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

In: Kerntechnik, Vol. 66, No. 1-2, 02.2001, p. 42-46.

Research output: Contribution to journal › Article

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title = "The astrophysical S-factor for dd-reactions at ke V-energy range",

abstract = "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.",

author = "V. Bystritskii and V. Bystritsky and S. Chaikovsky and M. Filipowicz and V. Grebenyuk and E. Gula and V. Makhrin and G. Mesyats and S. Parzhitski and F. Pen'Kov and N. Ratakhin and V. Sinebryukhov and S. Sorokin and V. Stolupin and E. Volkov and J. Wo{\'z}niak",

year = "2001",

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language = "English",

volume = "66",

pages = "42--46",

journal = "Kerntechnik",

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T1 - The astrophysical S-factor for dd-reactions at ke V-energy range

AU - Bystritskii, V.

AU - Bystritsky, V.

AU - Chaikovsky, S.

AU - Filipowicz, M.

AU - Grebenyuk, V.

AU - Gula, E.

AU - Makhrin, V.

AU - Mesyats, G.

AU - Parzhitski, S.

AU - Pen'Kov, F.

AU - Ratakhin, N.

AU - Sinebryukhov, V.

AU - Sorokin, S.

AU - Stolupin, V.

AU - Volkov, E.

AU - Woźniak, J.

PY - 2001/2

Y1 - 2001/2

N2 - 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.

AB - 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.

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