New Formula for Hydrogen Spectral Lines Wavelengths/Frequencies

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SUMMARY

The discussion presents a new formula for predicting the wavelengths and frequencies of hydrogen's spectral lines, derived using relativistic concepts. The formula, [cos(α/j) - cos(α/k)] * m * c^2, applies to transitions between energy levels j and k, where α is the fine structure constant, m is the mass of the electron, and c is the speed of light. This new approach shows that, similar to Bohr's original formula, it tends to overestimate transition energies, resulting in higher frequencies and lower wavelengths. The formula has been validated against measured values from HyperPhysics.

PREREQUISITES
  • Understanding of quantum mechanics and atomic transitions
  • Familiarity with the fine structure constant
  • Knowledge of relativistic physics concepts
  • Basic grasp of spectral line analysis
NEXT STEPS
  • Research the implications of the fine structure constant in quantum mechanics
  • Explore the derivation of Bohr's formula and its limitations
  • Learn about relativistic corrections in atomic physics
  • Investigate peer-reviewed literature on hydrogen spectral lines
USEFUL FOR

Physicists, researchers in quantum mechanics, and students studying atomic physics will benefit from this discussion, particularly those interested in spectral line analysis and relativistic effects in atomic transitions.

neilparker62
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Hi

I have a new formula (or at least I think it's new) for predicting the wavelengths/frequencies of hydrogen's spectral lines. Please take a look and tell me if it is new. I am quite confident that it works because Bohr's original formula 'falls out' if one approximates cos(x) as 1 + x^2/2 for small x. But the formula was derived by deploying some relativistic ideas without actually knowing much about relativity! Here is the energy expression for 1s to 2s transition. Translate to frequency or wavelength with the usual E=hf=hc/λ.

[cos(α/2) - cos(α)] * m * c^2

Where:

α = fine structure constant
m = mass of electron
c = velocity of light

More generally for level j to level k transitions:

[cos(α/j) - cos(α/k)] * m * c^2 (j > k).

I have checked this formula against a set of measured values I found here:

http://hyperphysics.phy-astr.gsu.edu/hbase/tables/hydspec.html#c1

Interesting that - like the Bohr formula - this formula seems to consistently overestimate transition energies thus leading to slightly higher than measured frequencies and conversely lower wavelengths.

I learned all about the 'fine structure constant' when developing this formula - it popped up again and again!
 
Physics news on Phys.org
New formulas should be published (along with their derivation and comparison to previous experiments) in the peer-reviewed literature. Not here on PF.
 

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