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光电离过程中Fe靶和V靶特征辐射的角相关研究

柳钰 徐忠锋 王兴 曾利霞 刘婷

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光电离过程中Fe靶和V靶特征辐射的角相关研究

柳钰, 徐忠锋, 王兴, 曾利霞, 刘婷

Angular distribution of characteristic X-ray emission from Fe and V following photoionization

Liu Yu, Xu Zhong-Feng, Wang Xing, Zeng Li-Xia, Liu Ting
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  • 在发射角120°—170°的范围内, 应用硅漂移探测器以10°为间隔对中心能量为13.1 keV的韧致辐射诱发Fe靶和V靶发射的典型K系X射线光谱进行了测量. 得到特征X射线KαKβ的特征谱线, 考虑探测器对特征X射线的探测效率、靶对入射光子和出射光子吸收的校准及大气对特征X射线的吸收后, 结果显示不同探测角度下KβKα的强度比为一常数. 将本次实验探测角度为150°时的Kβ/Kα强度比值的实验值、理论计算值和Ertuğral的实验结果进行对比, 发现实验结果与预期相符. 对比不同探测角度下的强度比变化趋势推断特征X射线的角度依赖关系, 分析认为KαKβ在探测范围内是各向同性发射的.
    The de-excitation process of vacancy in the inner shell of the target atom caused by collision ionization produces the characteristic X-ray or Auger electrons. The precise measurement of ionization cross sections plays an important role in many basic research fields, as well as in practical fields, such as chemical analysis of Particle Induced X-ray Emission (PIXE), atomic and nuclear processes, and X-ray fluorescence (XRF) spectroscopy. As we know, when ionization cross sections are measured precisely, whether the emission of X-ray is isotropic in collision process must be considered. However, there have been few experimental results for angular dependence of Kβ/Kα intensity ratios in the literature until now. Therefore, this study aims to verify that the Kα and Kβ X-rays originated from filling of the K shell vacancies with total angular momentum quantum number 1/2 (J = 1/2) are isotropic. In this work, the typical K-shell X-ray spectra for Fe and V, which induced by bremsstrahlung with central energy of 13.1 keV, have been measured at emission angles varied from 120° to 170° at intervals of 10°. The characteristic X-ray spectra obtained by the detector are fitted by Gauss function, where the absorption of incident X-rays by the detector, the absorption of emitted X-rays by the atmosphere and the self-absorption correction factor of incident and emitted X-rays by the target are all taken into account. The experimental results of Kβ/Kα intensity ratio in this experiment coincide with those of theoretical calculation, as well as the Ertuğral’s experimental result. The experimental results show that the intensity ratio of Kβ/Kα is a constant at different detection angles. Therefore it can be concluded that the emission of Kα and Kβ is isotropic in the detection range. Since the K shell has no sub-shell, there is no Coster-Kronig transition in the collision ionization process. In the process of photoionization, the vacancies in the K shell are produced by direct ionization. As a result, the cross section ratio of K shell X-ray generation is independent of the K shell photoionization cross section. In addition, the experimental results show that the Kβ/Kα characteristic X-ray intensity ratio of target Fe is 8% higher than that of target V, which are consistent with the theoretical analysis results that the characteristic X-ray intensity ratio depends on the target atomic number Z.
      通信作者: 柳钰, liuyuxianyang0625@126.com
    • 基金项目: 省部级-陕西省科技厅自然科学基础研究计划(2019JQ-493)
      Corresponding author: Liu Yu, liuyuxianyang0625@126.com
    [1]

    王兴, 赵永涛, 程锐, 周贤明, 徐戈, 孙渊博, 雷瑜, 王瑜玉, 任洁茹, 虞洋, 李永峰, 张小安, 李耀宗, 梁昌慧, 肖国青 2012 物理学报 61 193201Google Scholar

    Wang X, Zhao Y T, Cheng R, Zhou X M, Xu G, Sun Y B, Lei Y, Wang Y Y, Ren J R, Yu Y, Li Y F, Zhang X A, Li Y Z, Liang C H, Xiao G Q 2012 Acta Phys. Sin. 61 193201Google Scholar

    [2]

    Horvat V, Watson R L, Blackadar J M 2008 Phys. Rev. A 77 032724Google Scholar

    [3]

    梁昌慧, 张小安, 李耀宗, 赵永涛, 周贤明, 王兴, 梅策香, 肖国青 2018 物理学报 67 243201Google Scholar

    Liang C H, Zhang X A, Li Y Z, Zhao Y T, Zhou X M, Wang X, Mei C X, Xiao G Q 2018 Acta Phys. Sin. 67 243201Google Scholar

    [4]

    Han I, Şahin M, Demir L 2009 Appl. Radiat. Isot. 67 1027Google Scholar

    [5]

    Salem S, Stöhlker, T, Demian A B, Hagmann S, Kozhuharov C, Liesen D, Gumberidze A 2013 Phys. Rev. A 88 012701Google Scholar

    [6]

    Šmit Ž 2005 Nucl. Instrum. Methods B 240 258Google Scholar

    [7]

    Romo-Kröger C M 2010 Vacuum 84 1250Google Scholar

    [8]

    Ma K, Dong C Z, Xie L Y, Qu Y Z 2014 Chin. Phys.Lett. 31 103201Google Scholar

    [9]

    牟致栋, 魏琦瑛 2014 物理学报 63 083402Google Scholar

    Mu Z D, Wei Q Y 2014 Acta Phys. Sin. 63 083402Google Scholar

    [10]

    Freemantle C S, Sacks N, Topic M, Pineda-vargas C A 2014 Nucl. Instrum. Methods B 318 168Google Scholar

    [11]

    Kada W, Kishi A, Sueyasu M, Sato F, Kato Y, Iida T 2014 Nucl. Instrum. Methods B 318 51Google Scholar

    [12]

    Fernandez J E, Scot V, Verardi L, Salvat F 2014 Radiat. Phys. Chem. 95 22Google Scholar

    [13]

    Flugge S, Mehlhorn W, Schmidt V 1972 Phys. Rev. Lett. 29 7Google Scholar

    [14]

    马堃, 颉录有, 张登红, 董晨钟, 屈一至 2016 物理学报 65 083201Google Scholar

    Ma K, Xie L Y, Zhang D H, Dong C Z, Qu Y Z 2016 Acta Phys. Sin. 65 083201Google Scholar

    [15]

    Wang X, Xu Z F, Cheng L 2016 Radiat. Phys. Chem. 122 24Google Scholar

    [16]

    Slivinsky V W, Ebert P J 1969 Phys. Lett. A 29 463Google Scholar

    [17]

    Ertugrul M, Sogut O, Simsek O, Buyukkasap E 2001 J. Phys. B: At.Mol. Opt. Phys. 34 909Google Scholar

    [18]

    Richard P, Bonner T I, Furuta T, Morgan I L, Rhodes J R 1970 Phys. Rev. A 1 1044Google Scholar

    [19]

    Li T K, Watson R L 1974 Phys. Rev. A 9 1574Google Scholar

    [20]

    Salem S I, Wimmer R J 1970 Phys. Rev. A 2 1121Google Scholar

    [21]

    Yalçın P 2007 Nucl. Instrum. Methods B 254 182Google Scholar

    [22]

    Apaydın G, Aylıkcı V, Cengiz E, Kaya N, Kobya Y, Tıraşoğlu E 2008 Radiat. Phys. Chem. 77 923Google Scholar

    [23]

    Akkus T, Sahin Y, Yılmaz D, Tuzluca F N 2017 Can. J. Phys. 95 220Google Scholar

    [24]

    Ertuğral B, Apaydın G, Cevika U, Ertuğrul M, Kobya A I 2007 Radiat.Phys.Chem. 76 15Google Scholar

    [25]

    Scofield J H 1974 Phys. Rev. A 9 1041Google Scholar

    [26]

    Scofield J H 1974 At. Data Nucl. Data Tables 14 121Google Scholar

    [27]

    Manson S T, Kennedy D J 1974 At. Data Nucl. Data Tables 14 111Google Scholar

    [28]

    Berezhko E G, Kabachnik N M 1977 J. Phys. B: At.Mol. Opt. Phys. 10 2467Google Scholar

    [29]

    Kanaya K, Okayama S 1972 J. Phys. D: Appl. Phys. 5 43Google Scholar

    [30]

    Yadav N, Bhatt P, Singh R, Llovet X, Shanker R 2011 Appl. Radiat. Isot. 69 1380Google Scholar

  • 图 1  实验装置示意图

    Fig. 1.  Experimental setup.

    图 2  150°探测角下Fe靶和V靶的能谱分布图 (a) Fe靶; (b) V靶

    Fig. 2.  Characteristic K X-ray spectrum of Fe and V induced by impact with bremsstrahlung with central energy of 13.1 keV and measured at the emission angle of 150°: (a) Target Fe; (b) target V.

    图 3  探测角为120°—170°时, Fe靶和V靶特征X射线强度比Kβ/Kα的角分布关系

    Fig. 3.  Angular distribution of characteristic X-ray intensity ratios of Kβ/Kα at detection angles of 120°–170° for Fe and V.

    图 4  Kβ/Kα的实验值、Ertuğral[24]的实验结果和理论计算值[2527]对比图

    Fig. 4.  Comparison of X-ray intensity ratios Kβ/Kα in the present work, literature experimental results from Ertuğrul[24] and theoretical values[2527].

  • [1]

    王兴, 赵永涛, 程锐, 周贤明, 徐戈, 孙渊博, 雷瑜, 王瑜玉, 任洁茹, 虞洋, 李永峰, 张小安, 李耀宗, 梁昌慧, 肖国青 2012 物理学报 61 193201Google Scholar

    Wang X, Zhao Y T, Cheng R, Zhou X M, Xu G, Sun Y B, Lei Y, Wang Y Y, Ren J R, Yu Y, Li Y F, Zhang X A, Li Y Z, Liang C H, Xiao G Q 2012 Acta Phys. Sin. 61 193201Google Scholar

    [2]

    Horvat V, Watson R L, Blackadar J M 2008 Phys. Rev. A 77 032724Google Scholar

    [3]

    梁昌慧, 张小安, 李耀宗, 赵永涛, 周贤明, 王兴, 梅策香, 肖国青 2018 物理学报 67 243201Google Scholar

    Liang C H, Zhang X A, Li Y Z, Zhao Y T, Zhou X M, Wang X, Mei C X, Xiao G Q 2018 Acta Phys. Sin. 67 243201Google Scholar

    [4]

    Han I, Şahin M, Demir L 2009 Appl. Radiat. Isot. 67 1027Google Scholar

    [5]

    Salem S, Stöhlker, T, Demian A B, Hagmann S, Kozhuharov C, Liesen D, Gumberidze A 2013 Phys. Rev. A 88 012701Google Scholar

    [6]

    Šmit Ž 2005 Nucl. Instrum. Methods B 240 258Google Scholar

    [7]

    Romo-Kröger C M 2010 Vacuum 84 1250Google Scholar

    [8]

    Ma K, Dong C Z, Xie L Y, Qu Y Z 2014 Chin. Phys.Lett. 31 103201Google Scholar

    [9]

    牟致栋, 魏琦瑛 2014 物理学报 63 083402Google Scholar

    Mu Z D, Wei Q Y 2014 Acta Phys. Sin. 63 083402Google Scholar

    [10]

    Freemantle C S, Sacks N, Topic M, Pineda-vargas C A 2014 Nucl. Instrum. Methods B 318 168Google Scholar

    [11]

    Kada W, Kishi A, Sueyasu M, Sato F, Kato Y, Iida T 2014 Nucl. Instrum. Methods B 318 51Google Scholar

    [12]

    Fernandez J E, Scot V, Verardi L, Salvat F 2014 Radiat. Phys. Chem. 95 22Google Scholar

    [13]

    Flugge S, Mehlhorn W, Schmidt V 1972 Phys. Rev. Lett. 29 7Google Scholar

    [14]

    马堃, 颉录有, 张登红, 董晨钟, 屈一至 2016 物理学报 65 083201Google Scholar

    Ma K, Xie L Y, Zhang D H, Dong C Z, Qu Y Z 2016 Acta Phys. Sin. 65 083201Google Scholar

    [15]

    Wang X, Xu Z F, Cheng L 2016 Radiat. Phys. Chem. 122 24Google Scholar

    [16]

    Slivinsky V W, Ebert P J 1969 Phys. Lett. A 29 463Google Scholar

    [17]

    Ertugrul M, Sogut O, Simsek O, Buyukkasap E 2001 J. Phys. B: At.Mol. Opt. Phys. 34 909Google Scholar

    [18]

    Richard P, Bonner T I, Furuta T, Morgan I L, Rhodes J R 1970 Phys. Rev. A 1 1044Google Scholar

    [19]

    Li T K, Watson R L 1974 Phys. Rev. A 9 1574Google Scholar

    [20]

    Salem S I, Wimmer R J 1970 Phys. Rev. A 2 1121Google Scholar

    [21]

    Yalçın P 2007 Nucl. Instrum. Methods B 254 182Google Scholar

    [22]

    Apaydın G, Aylıkcı V, Cengiz E, Kaya N, Kobya Y, Tıraşoğlu E 2008 Radiat. Phys. Chem. 77 923Google Scholar

    [23]

    Akkus T, Sahin Y, Yılmaz D, Tuzluca F N 2017 Can. J. Phys. 95 220Google Scholar

    [24]

    Ertuğral B, Apaydın G, Cevika U, Ertuğrul M, Kobya A I 2007 Radiat.Phys.Chem. 76 15Google Scholar

    [25]

    Scofield J H 1974 Phys. Rev. A 9 1041Google Scholar

    [26]

    Scofield J H 1974 At. Data Nucl. Data Tables 14 121Google Scholar

    [27]

    Manson S T, Kennedy D J 1974 At. Data Nucl. Data Tables 14 111Google Scholar

    [28]

    Berezhko E G, Kabachnik N M 1977 J. Phys. B: At.Mol. Opt. Phys. 10 2467Google Scholar

    [29]

    Kanaya K, Okayama S 1972 J. Phys. D: Appl. Phys. 5 43Google Scholar

    [30]

    Yadav N, Bhatt P, Singh R, Llovet X, Shanker R 2011 Appl. Radiat. Isot. 69 1380Google Scholar

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出版历程
  • 收稿日期:  2019-10-09
  • 修回日期:  2019-12-16
  • 刊出日期:  2020-02-20

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