<span style="font-size:14.0pt;line-height: 115%;font-family:"Times New Roman";mso-fareast-font-family:"Times New Roman"; color:black;mso-ansi-language:EN-IN;mso-fareast-language:EN-IN;mso-bidi-language: HI" lang="EN-IN">Relative intensities of high energy Plasmon satellites in K_α X-ray <span style="font-size:14.0pt;line-height:115%; font-family:"Times New Roman";mso-fareast-font-family:HiddenHorzOCR;color:black; mso-ansi-language:EN-IN;mso-fareast-language:EN-IN;mso-bidi-language:HI" lang="EN-IN">emission spectra <span style="font-size:14.0pt;line-height:115%; font-family:"Times New Roman";mso-fareast-font-family:"Times New Roman"; color:black;mso-ansi-language:EN-IN;mso-fareast-language:EN-IN;mso-bidi-language: HI" lang="EN-IN">of various fluorine compounds</span></span></span>

Abstract

<span style="font-size:14.0pt;line-height: 115%;font-family:" times="" new="" roman";mso-fareast-font-family:"times="" roman";="" color:black;mso-ansi-language:en-in;mso-fareast-language:en-in;mso-bidi-language:="" hi"="" lang="EN-IN">The K¹L¹ satellites of <i>Kα</i>_1.2 X-ray emission line of various fluorine compounds may be identified as plasmon satellites. An explanation for their origin is suggested using the Bohm and Pines theory of plasma oscillations in solids. Present calculated values for the relative intensities of the K¹L¹ satellites with respect to the main <i>Kα</i>_1.2 X-ray line agree well with the experimentally observed values of Endo <i>et al., </i>[<i>Phys</i> <i>Rev A, </i>22 (1980) <span style="font-size:14.0pt;line-height:115%;font-family:" times="" new="" roman";="" mso-fareast-font-family:hiddenhorzocr;color:black;mso-ansi-language:en-in;="" mso-fareast-language:en-in;mso-bidi-language:hi"="" lang="EN-IN">1436 -1440].</span></span>