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

L. Dudkin Butakov, G. N. Dudkin, B. A. Nechaev, V. N. Padalko, A. V. Petrov, N. M. Polkovnikova, V. M. Bystritsky, V. V. Gerasimov, A. R. Krylov, S. S. Parzhitskii, V. M. Bystritskii, J. Wozniak

Research Nuclear Reactor Center

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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 E_col = 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	https://doi.org/10.3103/S1062873807110536
Publication status	Published - 1 Nov 2007

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ASJC Scopus subject areas

Physics and Astronomy(all)

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Butakov, L. D., Dudkin, G. N., Nechaev, B. A., Padalko, V. N., Petrov, A. V., Polkovnikova, N. M., ... Wozniak, J. (2007). 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. Bulletin of the Russian Academy of Sciences: Physics, 71(11), 1640-1645. https://doi.org/10.3103/S1062873807110536

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

Butakov, LD, Dudkin, GN , Nechaev, BA , Padalko, VN, Petrov, AV, Polkovnikova, NM, Bystritsky, VM, Gerasimov, VV, Krylov, AR, Parzhitskii, SS, Bystritskii, VM & Wozniak, J 2007, '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', Bulletin of the Russian Academy of Sciences: Physics, vol. 71, no. 11, pp. 1640-1645. https://doi.org/10.3103/S1062873807110536

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. / 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. In: Bulletin of the Russian Academy of Sciences: Physics. 2007 ; Vol. 71, No. 11. pp. 1640-1645.

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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.",

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10.3103/S1062873807110536