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首页> 外文期刊>Physics of particles and nuclei letters >Measuring the Astrophysical S Factors and the Cross Sections of the p(d, γ)~3He Reaction in the Ultralow Energy Region Using a Zirconium Deuteride Target
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Measuring the Astrophysical S Factors and the Cross Sections of the p(d, γ)~3He Reaction in the Ultralow Energy Region Using a Zirconium Deuteride Target

机译:使用氘化锆靶标测量超低能区内p(d,γ)〜3He反应的天体S因子和截面

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摘要

The present paper is dedicated to the study of the p(d, γ)~3He reaction mechanism with the use of a zirconium deuteride target at proton energies of 11–19 keV. The experiment has been carried out using a proton beam of a high-current pulsed Hall accelerator at the National Research Tomsk Polytechnic University. The dependences of the astrophysical S factor and the effective cross section of the pd reaction on the proton–deuteron collision energy are measured. The results were compared with the available data. The results detailed in the present work agree with the results of an experiment carried out by the LUNA collaboration with the use of a gaseous deuterium target.
机译:本文致力于以11–19 keV的质子能量使用氘化锆靶,研究p(d,γ)〜3He反应机理。该实验是使用国立托木斯克工业大学的高电流脉冲霍尔加速器的质子束进行的。测量了天文学的S因子和pd反应的有效截面对质子-氘核碰撞能的依赖性。将结果与可用数据进行比较。当前工作中详细介绍的结果与LUNA合作使用气态氘靶进行的​​实验结果吻合。

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