Preliminary results of the study of the d(d,n)<sup>3</sup>He reaction in the astrophysical energy range with the use of a Hall plasma accelerator

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

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., Bystritsky, V. M., Gerasimov, V. V., Krylov, A. R., Parzhitskii, S. S., Bystritskii, V. 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 › peer-review

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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title = "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",

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.",

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

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AU - Petrov, A. V.

AU - Polkovnikova, N. M.

AU - Bystritsky, V. M.

AU - Gerasimov, V. V.

AU - Krylov, A. R.

AU - Parzhitskii, S. S.

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AU - Wozniak, J.

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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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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

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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