Mathematica Yazılımı Kullanılarak Yakın Kızılötesi ve XUV Bölgesinde Asal Gazların Kırılma İndisi Değerlerinin Hesaplanması

Bu çalışmada, görünür, kızılötesi ve aşırı ultraviyole (XUV) bölgesindeki kırılma indisleri Mathematica yazılımı kullanılarak hesaplanmıştır. Atomik saçılma faktörleri yüksek foton enerji aralığı (20-60 eV) için simülasyonu gerçekleştirilmiştir. Atomik saçılma faktörleri kullanılarak kırılma indisi değerlerinin gerçek ve sanal kısmı, foton enerjisinin bir fonksiyonu olarak hesaplandı. Bu çalışmanın amacı, farklı dalga boyu bölgelerinde asal gazların kırılma indisini hesaplayan bir simülasyon programı sunmaktır. Yakın kızılötesi ve XUV bölgesindeki helyum (He), neon (Ne), argon (Ar) ve xenon (Xe) kırılma indisleri Mathematica yazılımı kullanılarak hesaplandı. Kırılma indisinin uygulama alanları bahsedilmiştir. Kırılma indislerini hesaplayan Mathematica programı Ek'te sunulmaktadır.

Computation of Refractive Index Values of Inert Gases at Near-Infrared and XUV Region Based on Mathematica Software

In this study, refractive indices in the visible, near-infrared, and extreme ultraviolet (XUV)regions are calculated based on Mathematica software. Atomic scattering factors are simulatedfor a high photon energy range (20-60 eV). By using the atomic scattering factors, the real andimaginary part of the index of refraction values are plotted as a function of photon energy. Thiswork aims to present a computational program, which calculates the index of refraction of theinert gases at different wavelength regions. The refractive indices of gases, namely helium (He),neon (Ne), argon (Ar), and xenon (Xe) in the near-infrared and XUV region are computed byusing Mathematica software. The applications of the index of refraction are discussed in the paper.The Mathematica program calculating the refractive indices is presented in the Appendix.

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