Alexander Fufaev
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Rydberg Formula: Understanding the Energy Spectrum of the Hydrogen Atom

Important Formula

Formula: Rydberg energy formula for H atom
What do the formula symbols mean?

Binding energy

Unit
Energy required to knock an electron, which is in the \( n \)-th state, out of the hydrogen atom. For example, the binding energy of the electron in the ground state is \( n = 1 \): \( 13.6 \, \mathrm{eV} \).

Quantum number

Unit
Principal quantum number is an integer indicating an energy level of the H atom. The electron in the H atom can occupy this energy state, which is characterized by \(n\).

Here is:

  • \( n = 1 \) is the ground state.
  • \( n = 2 \) is the first excited state.
  • \( n = 3 \) is the second excited state.
  • and so on...
Hydrogen atom - term diagram (energy levels)
Table of contents
  1. Important Formula
  2. Exercises with Solutions

The Rydberg formula describes the wavelengths \( \lambda\) of lines in the spectrum of the hydrogen atom. However, it also describes the discrete energy levels \( W\) of the hydrogen atom:

Hydrogen atom - term diagram (energy levels)

Exercises with Solutions

Use this formula eBook if you have problems with physics problems.

Exercise: Transition from \( n = 2 \) to \( n = 3 \) in the Hydrogen Atom

In the Bohr atomic model, consider the transition from the energy level \( n = 2 \) to \( n = 3 \).

  1. How much energy (in electron volts) does the electron need to move from the state \( n = 2 \) to a higher state \( n = 3 \)?
  2. What light frequency \( f \) can realize this transition?
  3. What wavelength \( \lambda \) corresponds to this frequency?
  4. What wavenumber \( k \) corresponds to this frequency?

Solution to Exercise #1.1

A transition of the electron from the energy level \( n = 2 \) to \( n = 3 \) corresponds to the so-called \( H_{\alpha} \) line in the hydrogen atom in the Bohr atomic model.

The binding energy of the electron in the state \( n = 2 \) is: $$ W_2 = \frac{-13.6 \, \text{eV}}{n^2} = \frac{-13.6 \, \text{eV}}{2^2} = -3.4 \, \text{eV} $$ Analogously for the binding energy in the state \( n = 3 \).

Accordingly, the electron needs the following amount of energy for the transition from \( n = 2 \) to \( n = 3 \): $$W_2 - W_3 = -3.4 \, \text{eV} - (-1.5 \, \text{eV}) = -1.9 \, \text{eV} $$

Solution to Task #1.2

To calculate the frequency of the photon capable of ensuring this transition, use the following relationship: $$ W = h \, f $$

The necessary energy \( W = |-1.9 \, \text{eV}| \) for the transition was calculated in part (a) of the task. So the required frequency \( f \) of the photon is: $$ f = \frac{E}{h} = \frac{ 1.9 \, \text{eV} }{ 6.6 \cdot10^{-34} \, \text{Js} } = \frac{ 1.9 \, \text{V} \cdot 1.6 \cdot 10^{-19} \, \text{As} }{ 6.6 \cdot 10^{-34} \, \text{Js} } = 4.6 \cdot 10^{14} \, \frac{1}{\text s} = 460 \, \text{THz} $$

Solution to Exercise #1.3

Each frequency \( f \) of a photon can also be assigned a wavelength \( \lambda \). The frequency and wavelength are linked by the speed of light \( c \): $$ \lambda = \frac{c}{f} = \frac{ 3 \cdot 10^8 \, \frac{\text m}{\text s} }{ 4.6 \cdot 10^{14} \, \frac{1}{\text s} } = 6.5 \cdot 10^{-7} \, \text{m} = 650 \cdot 10^{-9} \, \text{m} = 650 \, \text{nm}$$

Solution to Exercise #1.4

To illustrate how many times the photon with a wavelength \( \lambda = 650 \, \text{nm} \) (see task part 1.3) performs an oscillation per meter, you calculate the wavenumber: $$k = \frac{1}{\lambda} = \frac{1}{650 \cdot 10^{-9} \, \text{m} } = 1.5 \cdot 10^6 \, \frac{1}{\text m} $$