Astrophysical S factor for dd interaction at ultralow energies

Vit M. Bystritskiǐ, V. M. Bystritsky, S. A. Chaikovsky, M. Filipowicz, V. M. Grebenyuk, E. Guła, V. I. Makhrin, G. A. Mesyats, S. S. Parzhitski, F. M. Pen'kov, N. A. Ratakhin, V. A. Sinebryukhov, S. A. Sorokin, V. A. Stolupin, E. N. Volkov, J. Woźniak

Research output: Contribution to journalArticle

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Abstract

Experimental results are presented that were obtained by measuring the astrophysical S factor for dd interaction at very low deuteron collision energies by using the liner-plasma technique. The experiment was performed at the high-current generator of the High-Current Electronics Institute (Tomsk, Russia). The values found for the S factor at the deuteron collision energies of 1.80, 2.06, and 2.27 keV are Sdd = 114 ± 68, 64 ± 30, and 53 ± 16 keV b, respectively. The corresponding dd cross sections obtained as the product of the barrier factor and the measured astrophysical S factor are σndd(Ecol = 1.80 keV) = (4.3 ± 2.6) × 10-33cm2, σndd(Ecol = 2.06 keV) = (9.8 ± 4.6) × 10-33cm2, and σndd(Ecol = 2.27 keV) = (2.1 ± 0.6) × 10-32cm2.

Original languageEnglish
Pages (from-to)855-860
Number of pages6
JournalPhysics of Atomic Nuclei
Volume64
Issue number5
DOIs
Publication statusPublished - 1 May 2001
Externally publishedYes

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astrophysics
deuterons
high current
interactions
collisions
energy
linings
Russian Federation
generators
cross sections
products
electronics

ASJC Scopus subject areas

  • Atomic and Molecular Physics, and Optics
  • Nuclear and High Energy Physics

Cite this

Bystritskiǐ, V. M., Bystritsky, V. M., Chaikovsky, S. A., Filipowicz, M., Grebenyuk, V. M., Guła, E., ... Woźniak, J. (2001). Astrophysical S factor for dd interaction at ultralow energies. Physics of Atomic Nuclei, 64(5), 855-860. https://doi.org/10.1134/1.1378875

Astrophysical S factor for dd interaction at ultralow energies. / Bystritskiǐ, Vit M.; Bystritsky, V. M.; Chaikovsky, S. A.; Filipowicz, M.; Grebenyuk, V. M.; Guła, E.; Makhrin, V. I.; Mesyats, G. A.; Parzhitski, S. S.; Pen'kov, F. M.; Ratakhin, N. A.; Sinebryukhov, V. A.; Sorokin, S. A.; Stolupin, V. A.; Volkov, E. N.; Woźniak, J.

In: Physics of Atomic Nuclei, Vol. 64, No. 5, 01.05.2001, p. 855-860.

Research output: Contribution to journalArticle

Bystritskiǐ, VM, Bystritsky, VM, Chaikovsky, SA, Filipowicz, M, Grebenyuk, VM, Guła, E, Makhrin, VI, Mesyats, GA, Parzhitski, SS, Pen'kov, FM, Ratakhin, NA, Sinebryukhov, VA, Sorokin, SA, Stolupin, VA, Volkov, EN & Woźniak, J 2001, 'Astrophysical S factor for dd interaction at ultralow energies', Physics of Atomic Nuclei, vol. 64, no. 5, pp. 855-860. https://doi.org/10.1134/1.1378875
Bystritskiǐ VM, Bystritsky VM, Chaikovsky SA, Filipowicz M, Grebenyuk VM, Guła E et al. Astrophysical S factor for dd interaction at ultralow energies. Physics of Atomic Nuclei. 2001 May 1;64(5):855-860. https://doi.org/10.1134/1.1378875
Bystritskiǐ, Vit M. ; Bystritsky, V. M. ; Chaikovsky, S. A. ; Filipowicz, M. ; Grebenyuk, V. M. ; Guła, E. ; Makhrin, V. I. ; Mesyats, G. A. ; Parzhitski, S. S. ; Pen'kov, F. M. ; Ratakhin, N. A. ; Sinebryukhov, V. A. ; Sorokin, S. A. ; Stolupin, V. A. ; Volkov, E. N. ; Woźniak, J. / Astrophysical S factor for dd interaction at ultralow energies. In: Physics of Atomic Nuclei. 2001 ; Vol. 64, No. 5. pp. 855-860.
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abstract = "Experimental results are presented that were obtained by measuring the astrophysical S factor for dd interaction at very low deuteron collision energies by using the liner-plasma technique. The experiment was performed at the high-current generator of the High-Current Electronics Institute (Tomsk, Russia). The values found for the S factor at the deuteron collision energies of 1.80, 2.06, and 2.27 keV are Sdd = 114 ± 68, 64 ± 30, and 53 ± 16 keV b, respectively. The corresponding dd cross sections obtained as the product of the barrier factor and the measured astrophysical S factor are σndd(Ecol = 1.80 keV) = (4.3 ± 2.6) × 10-33cm2, σndd(Ecol = 2.06 keV) = (9.8 ± 4.6) × 10-33cm2, and σndd(Ecol = 2.27 keV) = (2.1 ± 0.6) × 10-32cm2.",
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N2 - Experimental results are presented that were obtained by measuring the astrophysical S factor for dd interaction at very low deuteron collision energies by using the liner-plasma technique. The experiment was performed at the high-current generator of the High-Current Electronics Institute (Tomsk, Russia). The values found for the S factor at the deuteron collision energies of 1.80, 2.06, and 2.27 keV are Sdd = 114 ± 68, 64 ± 30, and 53 ± 16 keV b, respectively. The corresponding dd cross sections obtained as the product of the barrier factor and the measured astrophysical S factor are σndd(Ecol = 1.80 keV) = (4.3 ± 2.6) × 10-33cm2, σndd(Ecol = 2.06 keV) = (9.8 ± 4.6) × 10-33cm2, and σndd(Ecol = 2.27 keV) = (2.1 ± 0.6) × 10-32cm2.

AB - Experimental results are presented that were obtained by measuring the astrophysical S factor for dd interaction at very low deuteron collision energies by using the liner-plasma technique. The experiment was performed at the high-current generator of the High-Current Electronics Institute (Tomsk, Russia). The values found for the S factor at the deuteron collision energies of 1.80, 2.06, and 2.27 keV are Sdd = 114 ± 68, 64 ± 30, and 53 ± 16 keV b, respectively. The corresponding dd cross sections obtained as the product of the barrier factor and the measured astrophysical S factor are σndd(Ecol = 1.80 keV) = (4.3 ± 2.6) × 10-33cm2, σndd(Ecol = 2.06 keV) = (9.8 ± 4.6) × 10-33cm2, and σndd(Ecol = 2.27 keV) = (2.1 ± 0.6) × 10-32cm2.

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