An atom or a molecule can absorb light and undergo a transition from one quantum state to another. The oscillator strength f_{12} of a transition from a lower state |1\rangle to an upper state |2\rangle may be defined by : f_{12} = \frac{2 }{3}\frac{m_e}{\hbar^2}(E_2 - E_1) \sum_{\alpha=x,y,z} | \langle 1 m_1 | R_\alpha | 2 m_2 \rangle |^2, where m_e is the mass of an electron and \hbar is the
reduced Planck constant. The
quantum states |n\rangle, n= 1,2, are assumed to have several degenerate sub-states, which are labeled by m_n. "Degenerate" means that they all have the same energy E_n. The operator R_x is the sum of the x-coordinates r_{i,x} of all N electrons in the system, i.e. : R_\alpha = \sum_{i=1}^N r_{i,\alpha}. The oscillator strength is the same for each sub-state |n m_n\rangle. The definition can be recast by inserting the
Rydberg energy \text{Ry} and
Bohr radius a_0 : f_{12} = \frac{E_2 - E_1}{3\, \text{Ry}} \frac{\sum_{\alpha=x,y,z} | \langle 1 m_1 | R_\alpha | 2 m_2 \rangle |^2}{a_0^2}. In case the matrix elements of R_x, R_y, R_z are the same, we can get rid of the sum and of the 1/3 factor : f_{12} = 2\frac{m_e}{\hbar^2}(E_2 - E_1) \, | \langle 1 m_1 | R_x | 2 m_2 \rangle |^2. == Thomas–Reiche–Kuhn sum rule ==