Lyman-Series: calculating the nuclear mass of an isotope

In summary, the Lyman-Series refers to the spectral lines emitted by hydrogen when electrons transition from higher energy levels to the first energy level (n=1). This series can be used to calculate the nuclear mass of an isotope by analyzing the wavelengths of emitted photons. The mass can be determined through the energy-mass equivalence principle, allowing for precise measurements of isotopes based on their spectral characteristics. The accuracy of these calculations is crucial for applications in nuclear physics and chemistry.
  • #1
LeoJakob
24
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Assuming I have a given wavelength λ of the hydrogen spectrum and I want to calculate the nuclear mass of the isotope, is my approach correct?

Rydberg-formula:

$$\frac{1}{\lambda} = R_M \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)$$

with $$R_M = \frac{R_\infty}{1 + \frac{m_e}{M}}$$

Setting ## n_1 = 1 ## and ##n_2 = 2 ##, we get:

$$\frac{1}{\lambda} = R_M \left( \frac{1}{1^2} - \frac{1}{2^2} \right)
\Leftrightarrow \frac{1}{\lambda} = R_M \left( 1 - \frac{1}{4} \right)
\Leftrightarrow \frac{1}{\lambda} = R_M \left( \frac{3}{4} \right)
\Leftrightarrow \frac{1}{\lambda} = \frac{3R_M}{4}
\Leftrightarrow R_M = \frac{4}{3\lambda}$$

Substituting ##R_M ##in the definition:

$$\frac{4}{3\lambda} = \frac{R_\infty}{1 + \frac{m_e}{M}}\Leftrightarrow 1 + \frac{m_e}{M} = \frac{3\lambda R_\infty}{4}\Leftrightarrow \frac{m_e}{M} = \frac{3\lambda R_\infty}{4} - 1 \Leftrightarrow M = \frac{m_e}{\frac{3\lambda R_\infty}{4} - 1}$$


Kind regards :)
 
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  • #2
Your calculations look correct to me.

However, your result for the nuclear mass ##M## will probably not be very accurate. The Rydberg formula is only approximate. A full quantum mechanical treatment of the hydrogen atom (including effects of relativity and electron spin) leads to a modification of your result that can be expressed as $$M = \frac{m_e}{\frac{3 \lambda R_{\infty}}{4}(1+\epsilon)-1}$$ where ##\epsilon## is a very small, dimensionless number that comes out of the long, messy calculation. ##\epsilon## is of the order of the square of the fine structure constant ##\alpha##. So ##\epsilon## is of the order of ##10^{-5}##.

At first, you might think that the very small value of ##\epsilon## would not make much difference in the calculation of ##M##. However, the denominator in the expression for ##M## is of the form ##x - 1## where ##x## is a number very close to 1. So, small changes in ##x## can make a big difference in ##M##.
 
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  • #3
I'm glad you answered I didn't see anything wrong either but I kept second guessing myself so chose to let someone else reply. Glad to see that at least I wasn't incorrect in both the answer and the choice of waiting to see if I was correct.
 
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