K. Amari , A. Kahoul , J.M. Sampaio , Y. Kasri , J.P. Marques , F. Parente , A. Hamidani , S. Croft , A. Favalli , S. Daoudi , A. Zidi , B. Berkani
{"title":"应用拟合方法编制经验和半经验Kα1、Kα2、Kβ1′和Kβ2′x射线荧光截面","authors":"K. Amari , A. Kahoul , J.M. Sampaio , Y. Kasri , J.P. Marques , F. Parente , A. Hamidani , S. Croft , A. Favalli , S. Daoudi , A. Zidi , B. Berkani","doi":"10.1016/j.jqsrt.2025.109393","DOIUrl":null,"url":null,"abstract":"<div><div>In this study, empirical and semi-empirical X-ray fluorescence cross-sections are generated for <span><math><mrow><mi>K</mi><msub><mi>α</mi><mn>1</mn></msub></mrow></math></span>, <span><math><mrow><mi>K</mi><msub><mi>α</mi><mn>2</mn></msub></mrow></math></span>, <span><math><mrow><mi>K</mi><mi>β</mi><msubsup><mrow></mrow><mn>1</mn><mo>′</mo></msubsup><mo>,</mo><mspace></mspace></mrow></math></span>and <span><math><mrow><mi>K</mi><mi>β</mi><msubsup><mrow></mrow><mn>2</mn><mo>′</mo></msubsup><mspace></mspace></mrow></math></span>lines. The approach used was the fitting of experimental data by three-dimensional formulae. The empirical values were obtained through a fitting method making use of a three-dimensional function against atomic number <em>Z</em> and excitation energy <em>E</em>, resulting in a three-dimensional plot allowing to estimate empirically <span><math><mrow><mi>K</mi><msub><mi>α</mi><mn>1</mn></msub></mrow></math></span>, <span><math><mrow><mi>K</mi><msub><mi>α</mi><mn>2</mn></msub></mrow></math></span>, <span><math><mrow><mi>K</mi><mi>β</mi><msubsup><mrow></mrow><mn>1</mn><mo>′</mo></msubsup></mrow></math></span>, and <span><math><mrow><mi>K</mi><mi>β</mi><msubsup><mrow></mrow><mn>2</mn><mo>′</mo></msubsup><mspace></mspace></mrow></math></span>X-ray fluorescence cross sections. Further, new semi-empirical values were derived by fitting the weighted average values using an analytical function against atomic number <em>Z</em> and energy <em>E</em>, and subsequently the ratio <span><math><mrow><msub><mi>S</mi><mi>W</mi></msub><mo>=</mo><msub><mrow><mo>(</mo><msub><mi>σ</mi><msub><mi>K</mi><mi>i</mi></msub></msub><mo>)</mo></mrow><mtext>exp</mtext></msub><mo>/</mo><msub><mrow><mo>(</mo><msub><mi>σ</mi><msub><mi>K</mi><mi>i</mi></msub></msub><mo>)</mo></mrow><mi>W</mi></msub><mspace></mspace></mrow></math></span>is fitted by a three-dimensional analyzing polynomial function as a function of <em>Z</em> and energy <em>E</em>. For <span><math><mrow><mi>K</mi><msub><mi>α</mi><mn>1</mn></msub></mrow></math></span> and <span><math><mrow><mi>K</mi><msub><mi>α</mi><mn>2</mn></msub></mrow></math></span> lines the range of atomic numbers covered was <span><math><mrow><mn>52</mn><mo>≤</mo><mi>Z</mi><mo>≤</mo><mn>92</mn></mrow></math></span> whereas for <span><math><mrow><mi>K</mi><mi>β</mi><msubsup><mrow></mrow><mn>1</mn><mo>′</mo></msubsup></mrow></math></span> and <span><math><mrow><mi>K</mi><mi>β</mi><msubsup><mrow></mrow><mn>2</mn><mo>′</mo></msubsup></mrow></math></span> it was<span><math><mrow><mspace></mspace><mn>57</mn><mo>≤</mo><mi>Z</mi><mo>≤</mo><mn>79</mn><mo>.</mo></mrow></math></span> Our findings were compared with selected experimental results, and good agreement was obtained.</div></div>","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"337 ","pages":"Article 109393"},"PeriodicalIF":2.3000,"publicationDate":"2025-02-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Compilation of empirical and semi-empirical Kα1, Kα2, Kβ1′, and Kβ2′ X-ray fluorescence cross-sections by the application of fitting approaches\",\"authors\":\"K. Amari , A. Kahoul , J.M. Sampaio , Y. Kasri , J.P. Marques , F. Parente , A. Hamidani , S. Croft , A. Favalli , S. Daoudi , A. Zidi , B. Berkani\",\"doi\":\"10.1016/j.jqsrt.2025.109393\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>In this study, empirical and semi-empirical X-ray fluorescence cross-sections are generated for <span><math><mrow><mi>K</mi><msub><mi>α</mi><mn>1</mn></msub></mrow></math></span>, <span><math><mrow><mi>K</mi><msub><mi>α</mi><mn>2</mn></msub></mrow></math></span>, <span><math><mrow><mi>K</mi><mi>β</mi><msubsup><mrow></mrow><mn>1</mn><mo>′</mo></msubsup><mo>,</mo><mspace></mspace></mrow></math></span>and <span><math><mrow><mi>K</mi><mi>β</mi><msubsup><mrow></mrow><mn>2</mn><mo>′</mo></msubsup><mspace></mspace></mrow></math></span>lines. The approach used was the fitting of experimental data by three-dimensional formulae. The empirical values were obtained through a fitting method making use of a three-dimensional function against atomic number <em>Z</em> and excitation energy <em>E</em>, resulting in a three-dimensional plot allowing to estimate empirically <span><math><mrow><mi>K</mi><msub><mi>α</mi><mn>1</mn></msub></mrow></math></span>, <span><math><mrow><mi>K</mi><msub><mi>α</mi><mn>2</mn></msub></mrow></math></span>, <span><math><mrow><mi>K</mi><mi>β</mi><msubsup><mrow></mrow><mn>1</mn><mo>′</mo></msubsup></mrow></math></span>, and <span><math><mrow><mi>K</mi><mi>β</mi><msubsup><mrow></mrow><mn>2</mn><mo>′</mo></msubsup><mspace></mspace></mrow></math></span>X-ray fluorescence cross sections. Further, new semi-empirical values were derived by fitting the weighted average values using an analytical function against atomic number <em>Z</em> and energy <em>E</em>, and subsequently the ratio <span><math><mrow><msub><mi>S</mi><mi>W</mi></msub><mo>=</mo><msub><mrow><mo>(</mo><msub><mi>σ</mi><msub><mi>K</mi><mi>i</mi></msub></msub><mo>)</mo></mrow><mtext>exp</mtext></msub><mo>/</mo><msub><mrow><mo>(</mo><msub><mi>σ</mi><msub><mi>K</mi><mi>i</mi></msub></msub><mo>)</mo></mrow><mi>W</mi></msub><mspace></mspace></mrow></math></span>is fitted by a three-dimensional analyzing polynomial function as a function of <em>Z</em> and energy <em>E</em>. For <span><math><mrow><mi>K</mi><msub><mi>α</mi><mn>1</mn></msub></mrow></math></span> and <span><math><mrow><mi>K</mi><msub><mi>α</mi><mn>2</mn></msub></mrow></math></span> lines the range of atomic numbers covered was <span><math><mrow><mn>52</mn><mo>≤</mo><mi>Z</mi><mo>≤</mo><mn>92</mn></mrow></math></span> whereas for <span><math><mrow><mi>K</mi><mi>β</mi><msubsup><mrow></mrow><mn>1</mn><mo>′</mo></msubsup></mrow></math></span> and <span><math><mrow><mi>K</mi><mi>β</mi><msubsup><mrow></mrow><mn>2</mn><mo>′</mo></msubsup></mrow></math></span> it was<span><math><mrow><mspace></mspace><mn>57</mn><mo>≤</mo><mi>Z</mi><mo>≤</mo><mn>79</mn><mo>.</mo></mrow></math></span> Our findings were compared with selected experimental results, and good agreement was obtained.</div></div>\",\"PeriodicalId\":16935,\"journal\":{\"name\":\"Journal of Quantitative Spectroscopy & Radiative Transfer\",\"volume\":\"337 \",\"pages\":\"Article 109393\"},\"PeriodicalIF\":2.3000,\"publicationDate\":\"2025-02-12\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Quantitative Spectroscopy & Radiative Transfer\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S002240732500055X\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"OPTICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Quantitative Spectroscopy & Radiative Transfer","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S002240732500055X","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"OPTICS","Score":null,"Total":0}
Compilation of empirical and semi-empirical Kα1, Kα2, Kβ1′, and Kβ2′ X-ray fluorescence cross-sections by the application of fitting approaches
In this study, empirical and semi-empirical X-ray fluorescence cross-sections are generated for , , and lines. The approach used was the fitting of experimental data by three-dimensional formulae. The empirical values were obtained through a fitting method making use of a three-dimensional function against atomic number Z and excitation energy E, resulting in a three-dimensional plot allowing to estimate empirically , , , and X-ray fluorescence cross sections. Further, new semi-empirical values were derived by fitting the weighted average values using an analytical function against atomic number Z and energy E, and subsequently the ratio is fitted by a three-dimensional analyzing polynomial function as a function of Z and energy E. For and lines the range of atomic numbers covered was whereas for and it was Our findings were compared with selected experimental results, and good agreement was obtained.
期刊介绍:
Papers with the following subject areas are suitable for publication in the Journal of Quantitative Spectroscopy and Radiative Transfer:
- Theoretical and experimental aspects of the spectra of atoms, molecules, ions, and plasmas.
- Spectral lineshape studies including models and computational algorithms.
- Atmospheric spectroscopy.
- Theoretical and experimental aspects of light scattering.
- Application of light scattering in particle characterization and remote sensing.
- Application of light scattering in biological sciences and medicine.
- Radiative transfer in absorbing, emitting, and scattering media.
- Radiative transfer in stochastic media.