用二次活化法和光谱法测量 9Be(d,xt)反应总截面

IF 0.48 Q4 Physics and Astronomy
L. N. Generalov, I. A. Karpov
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引用次数: 0

摘要

摘要根据 B.Ya. Guzhovskii 的方法,在全俄实验物理研究院(VNIIEF)的 EGP-10 型静电串联加速器上测量了 9Be(d,xt)反应的总截面 σd,xt,氘核能量范围在 1.5-12 МeV 之间,误差为 8.3%。Guzhovskii 的方法,在全俄实验物理研究院(VNIIEF)的 EGP-10 型静电串联加速器上进行的。主靶和转换器功能结合在 1 毫米厚的铍层中,如果铍层的厚度大于主氘核和次氚子路径的总和,就可以做到这一点。测量活化截面的主要问题是缺乏关于所考虑反应中产生的氚子平均能量的可靠数据。这个值是根据测量到的氚子能谱得出的。首次获得了光谱微分截面,并将其作为计算总反应截面的基础。总活化截面与光谱截面之间显示出良好的一致性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Measurement of the 9Be(d, xt) Reaction Total Cross Sections by Secondary Activation and Spectroscopy Methods

Measurement of the 9Be(d, xt) Reaction Total Cross Sections by Secondary Activation and Spectroscopy Methods

Measurement of the 9Be(d, xt) Reaction Total Cross Sections by Secondary Activation and Spectroscopy Methods

Total cross sections σd,xt of reaction 9Be(d, xt) are measured in the 1.5–12 МeV range of deuteron energies with an error of 8.3% using activation reaction 9Be + t → α + 8Li + 2.927 МeV (T1/2 = 0.84 s, Eβ max = 13 МeV) according to B.Ya. Guzhovskii’s method on the EGP-10 electrostatic tandem accelerator at the All-Russian Research Institute of Experimental Physics (VNIIEF). The primary target and convertor functions are combined in a beryllium layer 1 mm thick, which can be done if the layer is thicker than the sum of the paths of primary deuterons and secondary tritons. The main problem in measuring the cross sections of activation is the lack of reliable data on the mean energy of tritons produced in the considered reaction. This value is derived from measured triton energy spectra. Spectrometric differential cross sections are obtained for the first time and serve as the basis for calculating total reaction cross sections. Good agreement is shown between the total activation and spectrometric cross sections.

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来源期刊
Bulletin of the Russian Academy of Sciences: Physics
Bulletin of the Russian Academy of Sciences: Physics Physics and Astronomy-Physics and Astronomy (all)
CiteScore
0.90
自引率
0.00%
发文量
251
期刊介绍: Bulletin of the Russian Academy of Sciences: Physics is an international peer reviewed journal published with the participation of the Russian Academy of Sciences. It presents full-text articles (regular,  letters  to  the editor, reviews) with the most recent results in miscellaneous fields of physics and astronomy: nuclear physics, cosmic rays, condensed matter physics, plasma physics, optics and photonics, nanotechnologies, solar and astrophysics, physical applications in material sciences, life sciences, etc. Bulletin of the Russian Academy of Sciences: Physics  focuses on the most relevant multidisciplinary topics in natural sciences, both fundamental and applied. Manuscripts can be submitted in Russian and English languages and are subject to peer review. Accepted articles are usually combined in thematic issues on certain topics according to the journal editorial policy. Authors featured in the journal represent renowned scientific laboratories and institutes from different countries, including large international collaborations. There are globally recognized researchers among the authors: Nobel laureates and recipients of other awards, and members of national academies of sciences and international scientific societies.
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