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Visualized Solution
The Sigma Insight: Bohr's Atomic Model and Energy Levels
Visualizing the X-ray Transitions
Imagine you are looking at the energy levels of a hydrogen-like atom. When an electron jumps from a higher energy level to a lower one, it emits a photon. In the context of characteristic X-rays, these transitions have specific names. The line is emitted when an electron jumps from the L-shell () to the K-shell (). Similarly, the line is emitted when an electron jumps from the M-shell () to the K-shell ().
The Master Equation
Moseley's Law
To find the wavelength of these emitted X-rays, we rely on a combination of Moseley's Law and the Rydberg formula. The formula is given by:
Here, is the Rydberg constant, is the atomic number, and is the screening constant. For the K-series transitions, the screening constant is approximately . Since we are dealing with the same element for both transitions, the term remains constant. This means the wavelength is inversely proportional to the difference of the inverse squares of the principal quantum numbers:
Setting up the Ratio
By taking the ratio of the wavelengths of the and lines, we can eliminate the constant terms. The ratio is purely dependent on the quantum numbers:
Let's calculate the values inside the brackets. For the transition, we have . For the transition, we have . Substituting these back into our ratio gives:
Final Calculation
Simplifying the complex fraction, we get . Now, we can easily find the wavelength of the line by multiplying this fraction by the given wavelength of the line ():
Notice that the transition involves a larger energy difference than the transition. Because energy is inversely proportional to wavelength, it makes perfect sense that the wavelength is shorter than the wavelength. Always keep this physical intuition in mind to cross-check your answers!
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