首页> 外文期刊>Nuclear science and engineering >Angle-Dependent Double-Differential Neutron Emission Cross Sections of ~3H(t,n) Between 5.98 and 19.14 MeV and Evidence of ~4H as Intermediate Reaction Product
【24h】

Angle-Dependent Double-Differential Neutron Emission Cross Sections of ~3H(t,n) Between 5.98 and 19.14 MeV and Evidence of ~4H as Intermediate Reaction Product

机译:在3.98 MeV和19.14 MeV之间〜3H(t,n)的角度相关双微分中子发射截面和〜4H作为中间反应产物的证据

获取原文
获取原文并翻译 | 示例
       

摘要

Neutrons for fusion applications stem not only from monoenergetic sources but also from "white" neutron sources. In this regard, the reaction ~3H(t,n) is of particular interest. Continuous neutron spectra of the ~3H(t,n) reactions were measured at 5.98-, 7.47-, 10.45-, 16.41-, and 19.14-MeV triton energy at typically seven angles between 0 and 145 deg. The spectra at the three lowest energies contain only neutrons from ~3H(t,n)~5He and ~3H(t,2n)~4He reactions and therefore can more easily be interpreted than the spectra at 16.41 and 19.14 MeV, which are too complex to allow a straightforward decomposition except for estimation of the neutron emission cross section following the reaction ~3H(t,d)~4H. Angle-dependent double-differential and neutron energy-integrated cross sections are given at the five energies. In most cases the peak of the two-body ground state transition could be deconvolved reliably resulting in cross sections of the reaction ~3H(t,n)~5He. Although the basic scale uncertainty is <5%, severe background, in particular, at the higher triton energies, increases the total uncertainty of integrated cross sections up to 9%. Naturally, the uncertainty of each energy bin of the double-differential cross sections, which depend on bin width, is considerably higher. As no previous data are reported at or near these energies, no direct comparison with other data was feasible. Evidence is provided of the formation of the short-lived neutron-rich nuclei ~5He and at higher energies of ~4H.
机译:用于聚变的中子不仅来自单能源,而且还来自“白色”中子源。在这方面,反应〜3H(t,n)是特别令人感兴趣的。 〜3H(t,n)反应的连续中子光谱是在5.98-MeV,7.47-Me,10.45-Me,16.41-Me和19.14-MeV Triton能量下,通常在0至145度之间的七个角度测量的。三个最低能量的光谱仅包含〜3H(t,n)〜5He和〜3H(t,2n)〜4He反应的中子,因此比16.41和19.14 MeV的光谱更容易解释。除了估算〜3H(t,d)〜4H反应后的中子发射截面外,还可以进行简单分解。在五个能量处给出了角度相关的双微分和中子能量积分的截面。在大多数情况下,两体基态跃迁的峰可以可靠地解卷积,从而导致反应的横截面〜3H(t,n)〜5He。尽管基本尺度不确定度小于5%,但特别是在较高的Triton能量下,严重的背景会使积分截面的总不确定度增加至9%。自然地,取决于仓宽度,双微分横截面的每个能量仓的不确定性要高得多。由于没有报道过这些能量或接近这些能量的数据,因此无法与其他数据进行直接比较。有证据表明,短寿命的中子富核约为5He,能量约为4H。

著录项

相似文献

  • 外文文献
  • 中文文献
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号