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ATOMIC AND MOLECULAR PHOTOELECTRON SPECTROSCOPY STUDIES USING SYNCHROTRON RADIATION.

机译:使用同步加速器辐射进行原子和分子光电子谱研究。

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摘要

Using photons from the Canadian Synchrotron Radiation Facility (CSRF) at the Tantalus electron storage ring, gas phase photoelectron spectra of the Xe 4d(,3/2,5/2) core level, and the valence orbitals of CF(,4), SiF(,4), CF(,3)I, and XeF(,2) have been obtained as a function of photon energy. Theoretical branching ratios and partial cross sections obtained from MS-X(alpha) calculations, are compared with experiment for the molecular cases. These atomic and molecular systems were studied in order to further our understanding of shape resonances and many-body effects in photoionization.;Valence orbital branching ratios for CF(,4), SiF(,4), and CF(,3)I have been obtained from 21 to (TURN)100 eV photon energy. In general, the agreement between experiment and the MS-X(alpha) results is good. In contrast to the CF(,4) results which show little structure, five shape resonances are predicted for SiF(,4) at 3, 7, 13, 23, and 35 eV kinetic energies. Similarly, two shape resonances at 15 and 17 eV kinetic energies are predicted for CF(,3)I. Although much of the behavior of CF(,3)I is very similar to CF(,4), weak shape resonances at (TURN)13 eV kinetic energy have been observed on the 3e, 2e, and 1e orbitals. Intershell correlation effects in CF(,3)I have been found to occur above the I 4d edge on the I 5p lone pair orbital (4e).;Similarly, valence orbital branching ratios have been obtained for XeF(,2) from 21 to 50 eV photon energy. A number of strong resonances are predicted and observed, in spite of the apparent lack of appropriate valence virtual orbitals and the long bond distance.;The Xe 4d(,5/2):4d(,3/2) spin-orbit branching ratio has been accurately determined from 74 to 150 eV photon energy. There is good qualitative agreement between these values and the latest relativistic random-phase approximation (RRPA) calculations of Cheng and Johnson. It is proposed that deviations in the minimum region arise from the neglect of relaxation effects during photoionization.
机译:使用位于Tantalus电子存储环的加拿大同步辐射设施(CSRF)的光子,Xe 4d(,3 / 2,5 / 2)核心能级的气相光电子能谱以及CF(,4)的价态轨道,已获得SiF(,4),CF(,3)I和XeF(,2)作为光子能量的函数。从MS-Xα计算得到的理论支化比和部分截面与分子情况的实验进行了比较。对这些原子和分子系统进行了研究,以进一步了解光电离中的形状共振和多体效应。CF(,4),SiF(,4)和CF(,3)I的价轨道支化比为从21到(TURN)100 eV光子能量获得通常,实验与MS-Xα结果之间的一致性很好。与显示很少结构的CF(,4)结果相反,SiF(,4)在3、7、13、23和35 eV动能下预测了五个形状共振。同样,对于CF(,3)I,预测了在15和17 eV动能下的两个形状共振。尽管CF(,3)I的许多行为与CF(,4)非常相似,但在3e,2e和1e轨道上观察到了(TURN)13 eV动能的弱形状共振。已发现CF(,3)I中的壳间相关效应发生在I 5p孤对轨道(4e)的I 4d边缘上方。类似地,XeF(,2)的价轨道分支比已从21降低至21。 50 eV光子能量。尽管明显缺乏适当的化合价虚拟轨道和较长的键距,但仍预测并观察到许多强共振。Xe 4d(,5/2):4d(,3/2)自旋轨道分支比已经精确地确定了74至150 eV的光子能量。这些值与Cheng和Johnson的最新相对论随机相位近似(RRPA)计算之间有很好的定性一致性。建议最小区域中的偏差是由于在光电离过程中忽略弛豫效应而引起的。

著录项

  • 作者

    YATES, BRIAN WAYNE.;

  • 作者单位

    The University of Western Ontario (Canada).;

  • 授予单位 The University of Western Ontario (Canada).;
  • 学科 Physical chemistry.
  • 学位 Ph.D.
  • 年度 1986
  • 页码 1 p.
  • 总页数 1
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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