In X-ray diffraction, the Rachinger correction is a method for accounting for the effect of an undesired K-alpha 2 peak in the energy spectrum. Ideally, diffraction measurements are made with X-rays of a single wavelength. Practically, the x-rays for a measurement are usually generated in an X-ray tube from a metal's K-alpha line. This generation creates x-rays at a variety of wavelengths, but most of the non K-alpha X-rays can be blocked from reaching the sample by filters. However, the K-alpha line is actually two x-ray lines close together: the stronger K-alpha 1 peak, and the weaker K-alpha 2 peak. Compared to other radiation such as the Bremsstrahlung, the K-alpha two peak is more difficult to filter mechanically. The Rachinger correction is a recursive method suggested by William Albert Rachinger (1927) to eliminate the disturbing K α 2 {\displaystyle K_{\alpha _{2}}} peak.
Cause of the double peak For diffraction experiments with X-rays radiation is usually used with the K α {\displaystyle K_{\alpha }} Wavelength of the anode material . However, this is a doublet, so in reality two slightly different wavelengths. According to the diffraction conditions of the Laue or Bragg equation, both wavelengths each generate an intensity maximum. These maxima are very close to each other, with their distance depending on the diffraction angle 2 θ {\displaystyle 2\theta } . For larger angles, the distance of the intensity maxima is greater.
Procedure
Basics The wavelengths of K α 1 {\displaystyle K_{\alpha _{1}}} and K α 2 {\displaystyle K_{\alpha _{2}}} radiation are also known to increase their energy through the relationship:
E = h c 0 λ {\displaystyle E=h{\frac {c_{0}}{\lambda }}}
From this, the angular distance can be determined for each diffraction angle Δ θ {\displaystyle \Delta \theta } determine the two Kα peaks. Furthermore, it is known how the intensities of K α 1 {\displaystyle K_{\alpha _{1}}} and K α 2 {\displaystyle K_{\alpha _{2}}} behave in the diffraction pattern. This ratio is determined quantum mechanically and is for all anode materials:
r = I α 2 I α 1 = 0.5 {\displaystyle r={\frac {I_{\alpha _{2}}}{I_{\alpha _{1}}}}=0.5}
Calculation The total intensity is:
I ( θ ) = I 1 ( θ ) + I 2 ( θ ) {\displaystyle I(\theta )=I_{1}(\theta )+I_{2}(\theta )} , where I 1 ( θ ) {\displaystyle I_{1}(\theta )} is the intensity of the pure K α 1 {\displaystyle K_{\alpha _{1}}} peak and I 2 ( θ ) {\displaystyle I_{2}(\theta )} the intensity of the pure α 2 {\displaystyle \alpha _{2}} peak. The intensity of K α 2 {\displaystyle K_{\alpha _{2}}} peak can be expressed as:
I 2 ( θ ) = r ⋅ I 1 ( θ − Δ θ ) {\displaystyle I_{2}(\theta )=r\cdot I_{1}(\theta -\Delta \theta )} , so the overall intensity is:
I ( θ ) = I 1 ( θ ) + r ⋅ I 1 ( θ − Δ θ ) {\displaystyle I(\theta )=I_{1}(\theta )+r\cdot I_{1}(\theta -\Delta \theta )}
Practical Implementation
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