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 language | English |
|---|---|
| Pages (from-to) | 855-860 |
| Number of pages | 6 |
| Journal | Physics of Atomic Nuclei |
| Volume | 64 |
| Issue number | 5 |
| DOIs | |
| Publication status | Published - 1 May 2001 |
| Externally published | Yes |
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ASJC Scopus subject areas
- Atomic and Molecular Physics, and Optics
- Nuclear and High Energy Physics
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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 journal › Article
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TY - JOUR
T1 - Astrophysical S factor for dd interaction at ultralow energies
AU - Bystritskiǐ, Vit M.
AU - Bystritsky, V. M.
AU - Chaikovsky, S. A.
AU - Filipowicz, M.
AU - Grebenyuk, V. M.
AU - Guła, E.
AU - Makhrin, V. I.
AU - Mesyats, G. A.
AU - Parzhitski, S. S.
AU - Pen'kov, F. M.
AU - Ratakhin, N. A.
AU - Sinebryukhov, V. A.
AU - Sorokin, S. A.
AU - Stolupin, V. A.
AU - Volkov, E. N.
AU - Woźniak, J.
PY - 2001/5/1
Y1 - 2001/5/1
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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U2 - 10.1134/1.1378875
DO - 10.1134/1.1378875
M3 - Article
VL - 64
SP - 855
EP - 860
JO - Physics of Atomic Nuclei
JF - Physics of Atomic Nuclei
SN - 1063-7788
IS - 5
ER -