On the Intensities of X-Ray Kα Satellites of Neon

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概要

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• The origin of Kα satellites was generally believed to be one electron transition (1s→2p) between doubly ionized states 1s2s→2s2p and 1s2p→2p2p. It was assumed that these ionizations take place due to, rather than formerly supposed direct collisions, the electron shake-off processes by a sudden change of the effective nuclear charge just after the ejection of K electron from the atom, which is subject to an impinging electron or X-ray photon. The ratio of the probabilities for occurrence of a 1s2p state to 1s2s state is calculated for neon by sudden approximation. On the other hand, by using the theory for the line strengths of multiplets and experimental data of X-ray spectra, this ratio is also computed. These two values coincide with each other, if a reasonable small value (almost zero) is chosen for the Coster-Kronig yield.

• 社団法人日本物理学会の論文
• 1967-10-05

著者

• Sawada Masao

  Department Of Physics Faculty Of Science Osaka University

• Sawada Masao

  Department Of Solid Slate Physics Osaka Electro-communication University

関連論文

• On the Amorphous State of the Binary System of Nickel-Sulfur
• Fine Structures of X-ray K AbSorption Spectra of Copper in Various Copper Compounds
• Fine Structures of X-ray Absorption Spectra Of Cobalt in the Face Centered Cubic Lattice and Close-packed Hexagonal Lattice
• The Input Power Limit of the Cylindrical Rotating Anode of a X-ray Tube
• Fine Structures of X-ray Absorption Spectra of Crystalline and Amorphous Germanium
• On the Intensities of X-Ray Kα Satellites of Neon
• On the Structure of the X-Ray Non-diagram Lines Kβ_η for Elements from Cr(24) to Zn(30)
• On the Fine Structures of X-ray Absorption Spectra of Amorphous Substances : The Amorphous State of the Binary System of Nickel-Sulfur. II.

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