Investigation of the D(3He, p)4He Reaction in the Astrophysical Energy Region of 18 ÷ 30 keV

Abstract

The D(³He, p)⁴He reaction is first investigated in a solid target of deuterated zirconium (ZrD) in the ³He⁺ ion energy range E_He = 18 ÷ 30 keV (E = 7.212.0 keV in the center-of-mass system) with a step of 2 keV. The electron screening potential U_e = 617.8 ± 154.7 eV and the D(³He, p)⁴He reaction enhancement factors are experimentally determined in the given energy range. The measured electron screening potential is six times higher than in gaseous targets. This can be due to the ZrD lattice effects, which have not been studied either theoretically or experimentally so far. The D(³He, p)⁴He reaction has been investigated at the pulsed plasma Hall accelerator (Tomsk).

Original language	English
Pages (from-to)	1-6
Number of pages	6
Journal	JETP Letters
DOIs	https://doi.org/10.1134/S0021364018110012
Publication status	Accepted/In press - 28 May 2018

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

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@article{a7de3bedf23f4c91bcd531edf2c62a08,

title = "Investigation of the D(3He, p)4He Reaction in the Astrophysical Energy Region of 18 ÷ 30 keV",

abstract = "The D(3He, p)4He reaction is first investigated in a solid target of deuterated zirconium (ZrD) in the 3He+ ion energy range EHe = 18 ÷ 30 keV (E = 7.212.0 keV in the center-of-mass system) with a step of 2 keV. The electron screening potential Ue = 617.8 ± 154.7 eV and the D(3He, p)4He reaction enhancement factors are experimentally determined in the given energy range. The measured electron screening potential is six times higher than in gaseous targets. This can be due to the ZrD lattice effects, which have not been studied either theoretically or experimentally so far. The D(3He, p)4He reaction has been investigated at the pulsed plasma Hall accelerator (Tomsk).",

author = "Bystritsky, {V. M.} and Dudkin, {G. N.} and Nechaev, {B. A.} and Padalko, {V. N.} and Pen{\textquoteright}kov, {F. M.} and Tuleushev, {Y. Z.} and M. Filipowicz and Philippov, {A. V.}",

year = "2018",

month = may,

day = "28",

doi = "10.1134/S0021364018110012",

language = "English",

pages = "1--6",

journal = "JETP Letters",

issn = "0021-3640",

publisher = "Maik Nauka-Interperiodica Publishing",

}

TY - JOUR

T1 - Investigation of the D(3He, p)4He Reaction in the Astrophysical Energy Region of 18 ÷ 30 keV

AU - Bystritsky, V. M.

AU - Dudkin, G. N.

AU - Nechaev, B. A.

AU - Padalko, V. N.

AU - Pen’kov, F. M.

AU - Tuleushev, Y. Z.

AU - Filipowicz, M.

AU - Philippov, A. V.

PY - 2018/5/28

Y1 - 2018/5/28

N2 - The D(3He, p)4He reaction is first investigated in a solid target of deuterated zirconium (ZrD) in the 3He+ ion energy range EHe = 18 ÷ 30 keV (E = 7.212.0 keV in the center-of-mass system) with a step of 2 keV. The electron screening potential Ue = 617.8 ± 154.7 eV and the D(3He, p)4He reaction enhancement factors are experimentally determined in the given energy range. The measured electron screening potential is six times higher than in gaseous targets. This can be due to the ZrD lattice effects, which have not been studied either theoretically or experimentally so far. The D(3He, p)4He reaction has been investigated at the pulsed plasma Hall accelerator (Tomsk).

AB - The D(3He, p)4He reaction is first investigated in a solid target of deuterated zirconium (ZrD) in the 3He+ ion energy range EHe = 18 ÷ 30 keV (E = 7.212.0 keV in the center-of-mass system) with a step of 2 keV. The electron screening potential Ue = 617.8 ± 154.7 eV and the D(3He, p)4He reaction enhancement factors are experimentally determined in the given energy range. The measured electron screening potential is six times higher than in gaseous targets. This can be due to the ZrD lattice effects, which have not been studied either theoretically or experimentally so far. The D(3He, p)4He reaction has been investigated at the pulsed plasma Hall accelerator (Tomsk).

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DO - 10.1134/S0021364018110012

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JO - JETP Letters

JF - JETP Letters

SN - 0021-3640

ER -

Investigation of the D(³He, p)⁴He Reaction in the Astrophysical Energy Region of 18 ÷ 30 keV

Abstract

ASJC Scopus subject areas

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