K. Amari , A. Kahoul , J.M. Sampaio , S. Daoudi , J.P. Marques , F. Parente , A. Hamidani , S. Croft , A. Favalli , Y. Kasri , A. Zidi , B. Berkani
{"title":"用三维半经验公式计算5.46 ~ 123.6keV光子k壳层x射线荧光截面","authors":"K. Amari , A. Kahoul , J.M. Sampaio , S. Daoudi , J.P. Marques , F. Parente , A. Hamidani , S. Croft , A. Favalli , Y. Kasri , A. Zidi , B. Berkani","doi":"10.1016/j.jqsrt.2025.109479","DOIUrl":null,"url":null,"abstract":"<div><div>In this work, we propose a novel three-dimensional semi-empirical formula for the estimation of K-shell X-ray fluorescence cross sections for a wide range of elements <span><math><mrow><mn>16</mn><mo>≤</mo><mi>Z</mi><mo>≤</mo><mn>92</mn></mrow></math></span> based on the database of the experimental values published between 1985 and 2023 for photons spanning from 5.46 to 123.6 keV (over 3300 data). This approach employs an analytical dependent on the atomic number Z and the energy E. Subsequently, the ratio <span><math><mrow><msub><mi>S</mi><mi>W</mi></msub><mo>=</mo><mrow><mo>(</mo><msub><mi>σ</mi><mrow><mi>K</mi><mi>i</mi><mo>−</mo><mi>E</mi><mi>x</mi><mi>p</mi></mrow></msub><mo>)</mo></mrow><mo>/</mo><mrow><mo>(</mo><msub><mi>σ</mi><mrow><mi>K</mi><mi>i</mi><mo>−</mo><mi>W</mi></mrow></msub><mo>)</mo></mrow></mrow></math></span> are fitted using a three-dimension polynomial function, in terms of the atomic number Z and energy E. The cross-sections were described as the product of two functions, the first is a polynomial that represents the weighted mean of cross-sections values across different conditions and the second function provides additional fitting to the cross-section based on atomic numbers Z and energy E. The cross-sections expressed as function of these two variables show reasonable agreement with the experimental values.</div></div>","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"342 ","pages":"Article 109479"},"PeriodicalIF":2.3000,"publicationDate":"2025-04-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Computation of K-shell X-ray Fluorescence Cross Section for photons ranging from 5.46keV to 123.6keV using three-dimensional semi-empirical formulae\",\"authors\":\"K. Amari , A. Kahoul , J.M. Sampaio , S. Daoudi , J.P. Marques , F. Parente , A. Hamidani , S. Croft , A. Favalli , Y. Kasri , A. Zidi , B. Berkani\",\"doi\":\"10.1016/j.jqsrt.2025.109479\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>In this work, we propose a novel three-dimensional semi-empirical formula for the estimation of K-shell X-ray fluorescence cross sections for a wide range of elements <span><math><mrow><mn>16</mn><mo>≤</mo><mi>Z</mi><mo>≤</mo><mn>92</mn></mrow></math></span> based on the database of the experimental values published between 1985 and 2023 for photons spanning from 5.46 to 123.6 keV (over 3300 data). This approach employs an analytical dependent on the atomic number Z and the energy E. Subsequently, the ratio <span><math><mrow><msub><mi>S</mi><mi>W</mi></msub><mo>=</mo><mrow><mo>(</mo><msub><mi>σ</mi><mrow><mi>K</mi><mi>i</mi><mo>−</mo><mi>E</mi><mi>x</mi><mi>p</mi></mrow></msub><mo>)</mo></mrow><mo>/</mo><mrow><mo>(</mo><msub><mi>σ</mi><mrow><mi>K</mi><mi>i</mi><mo>−</mo><mi>W</mi></mrow></msub><mo>)</mo></mrow></mrow></math></span> are fitted using a three-dimension polynomial function, in terms of the atomic number Z and energy E. The cross-sections were described as the product of two functions, the first is a polynomial that represents the weighted mean of cross-sections values across different conditions and the second function provides additional fitting to the cross-section based on atomic numbers Z and energy E. The cross-sections expressed as function of these two variables show reasonable agreement with the experimental values.</div></div>\",\"PeriodicalId\":16935,\"journal\":{\"name\":\"Journal of Quantitative Spectroscopy & Radiative Transfer\",\"volume\":\"342 \",\"pages\":\"Article 109479\"},\"PeriodicalIF\":2.3000,\"publicationDate\":\"2025-04-16\",\"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/S0022407325001414\",\"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/S0022407325001414","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}
Computation of K-shell X-ray Fluorescence Cross Section for photons ranging from 5.46keV to 123.6keV using three-dimensional semi-empirical formulae
In this work, we propose a novel three-dimensional semi-empirical formula for the estimation of K-shell X-ray fluorescence cross sections for a wide range of elements based on the database of the experimental values published between 1985 and 2023 for photons spanning from 5.46 to 123.6 keV (over 3300 data). This approach employs an analytical dependent on the atomic number Z and the energy E. Subsequently, the ratio are fitted using a three-dimension polynomial function, in terms of the atomic number Z and energy E. The cross-sections were described as the product of two functions, the first is a polynomial that represents the weighted mean of cross-sections values across different conditions and the second function provides additional fitting to the cross-section based on atomic numbers Z and energy E. The cross-sections expressed as function of these two variables show reasonable agreement with the experimental values.
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.