Abstract
The possibility of using a plasma accelerator based on a pulsed Hall ion source to study the characteristics of pd, dd, d3He, 3He, and4He reactions in the astrophysical energy range (2-12 keV) has been considered. The preliminary experimental data on measurement of the astrophysical S factor for the dd reaction (dd → 3He + n (2.5 MeV)) at average deuteron collision energies Ecol = 4.5 and 4.95 keV and the deuteron beam energy spread FWHM = 18% are reported. The found value of the S factor is in agreement with the results of the experiments carried out by us previously using linear plasma in the inverse Z-pinch configuration.
| Original language | English |
|---|---|
| Pages (from-to) | 1640-1645 |
| Number of pages | 6 |
| Journal | Bulletin of the Russian Academy of Sciences: Physics |
| Volume | 71 |
| Issue number | 11 |
| DOIs | |
| Publication status | Published - 1 Nov 2007 |
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ASJC Scopus subject areas
- Physics and Astronomy(all)
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Preliminary results of the study of the d(d,n)3He reaction in the astrophysical energy range with the use of a Hall plasma accelerator. / Butakov, L. Dudkin; Dudkin, G. N.; Nechaev, B. A.; Padalko, V. N.; Petrov, A. V.; Polkovnikova, N. M.; Bystritsky, V. M.; Gerasimov, V. V.; Krylov, A. R.; Parzhitskii, S. S.; Bystritskii, V. M.; Wozniak, J.
In: Bulletin of the Russian Academy of Sciences: Physics, Vol. 71, No. 11, 01.11.2007, p. 1640-1645.Research output: Contribution to journal › Article
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TY - JOUR
T1 - Preliminary results of the study of the d(d,n)3He reaction in the astrophysical energy range with the use of a Hall plasma accelerator
AU - Butakov, L. Dudkin
AU - Dudkin, G. N.
AU - Nechaev, B. A.
AU - Padalko, V. N.
AU - Petrov, A. V.
AU - Polkovnikova, N. M.
AU - Bystritsky, V. M.
AU - Gerasimov, V. V.
AU - Krylov, A. R.
AU - Parzhitskii, S. S.
AU - Bystritskii, V. M.
AU - Wozniak, J.
PY - 2007/11/1
Y1 - 2007/11/1
N2 - The possibility of using a plasma accelerator based on a pulsed Hall ion source to study the characteristics of pd, dd, d3He, 3He, and4He reactions in the astrophysical energy range (2-12 keV) has been considered. The preliminary experimental data on measurement of the astrophysical S factor for the dd reaction (dd → 3He + n (2.5 MeV)) at average deuteron collision energies Ecol = 4.5 and 4.95 keV and the deuteron beam energy spread FWHM = 18% are reported. The found value of the S factor is in agreement with the results of the experiments carried out by us previously using linear plasma in the inverse Z-pinch configuration.
AB - The possibility of using a plasma accelerator based on a pulsed Hall ion source to study the characteristics of pd, dd, d3He, 3He, and4He reactions in the astrophysical energy range (2-12 keV) has been considered. The preliminary experimental data on measurement of the astrophysical S factor for the dd reaction (dd → 3He + n (2.5 MeV)) at average deuteron collision energies Ecol = 4.5 and 4.95 keV and the deuteron beam energy spread FWHM = 18% are reported. The found value of the S factor is in agreement with the results of the experiments carried out by us previously using linear plasma in the inverse Z-pinch configuration.
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U2 - 10.3103/S1062873807110536
DO - 10.3103/S1062873807110536
M3 - Article
AN - SCOPUS:37349095242
VL - 71
SP - 1640
EP - 1645
JO - Bulletin of the Russian Academy of Sciences: Physics
JF - Bulletin of the Russian Academy of Sciences: Physics
SN - 1062-8738
IS - 11
ER -