{"title":"Internal conversion tables part I: K-, L-, M-shell conversion coefficients for Z=30 to Z=103","authors":"R.S. Hager, E.C. Seltzer","doi":"10.1016/S0550-306X(68)80002-3","DOIUrl":null,"url":null,"abstract":"<div><p>Values of the internal conversion coefficient, number of electrons per photon emitted in a nuclear transition, are presented from a new relativistic self-consistent-field calculation which takes into account finite nuclear size, hole and exchange effects, experimental electron binding energies, and vacuum polarization. Coefficients are given for each value of <em>Z</em>; for <em>K, L</em>, and <em>M</em> electron shells and <em>L</em>- and <em>M</em>-sub-shells; for nuclear-transition multipolarities E1…E4, M1…M4; and for various nuclear-transition energies up to 1500 keV. A program for finding values for other energies by spline interpolation is appended.</p></div>","PeriodicalId":100967,"journal":{"name":"Nuclear Data Sheets. Section A","volume":"4 1","pages":"Pages 1-11"},"PeriodicalIF":0.0000,"publicationDate":"1968-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S0550-306X(68)80002-3","citationCount":"974","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Nuclear Data Sheets. Section A","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0550306X68800023","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 974
Abstract
Values of the internal conversion coefficient, number of electrons per photon emitted in a nuclear transition, are presented from a new relativistic self-consistent-field calculation which takes into account finite nuclear size, hole and exchange effects, experimental electron binding energies, and vacuum polarization. Coefficients are given for each value of Z; for K, L, and M electron shells and L- and M-sub-shells; for nuclear-transition multipolarities E1…E4, M1…M4; and for various nuclear-transition energies up to 1500 keV. A program for finding values for other energies by spline interpolation is appended.