Line Spectra and De Broglie's Explanation
The Line Spectra Of The Hydrogen Atom (Calculation of Wavelengths)
As discussed earlier (Section I2 of Rutherford's Model and Atomic Spectra), the emission and absorption spectra of hydrogen consist of discrete lines at specific wavelengths. Bohr's model successfully explained the origin of these lines based on electron transitions between quantised energy levels.
Energy Levels of Hydrogen
According to Bohr's model, the allowed energy levels of the electron in a hydrogen atom ($Z=1$) are given by:
$ E_n = -\frac{13.6}{n^2} \, eV $
Where $n=1, 2, 3, ...$ are the principal quantum numbers. $E_1$ is the energy of the ground state, $E_2$ is the energy of the first excited state, and so on.
Calculation of Wavelengths of Spectral Lines
According to Bohr's third postulate, a spectral line is emitted when an electron makes a transition from a higher energy level $E_{n_i}$ (corresponding to quantum number $n_i$) to a lower energy level $E_{n_f}$ (corresponding to quantum number $n_f$), where $n_i > n_f$. The energy of the emitted photon ($h\nu$) is equal to the difference in the energies of the initial and final levels:
$ h\nu = E_{n_i} - E_{n_f} $
Substitute the energy formula $E_n = -\frac{13.6}{n^2}$:
$ h\nu = \left(-\frac{13.6}{n_i^2}\right) - \left(-\frac{13.6}{n_f^2}\right) $
$ h\nu = 13.6 \left(\frac{1}{n_f^2} - \frac{1}{n_i^2}\right) \, eV $
The frequency $\nu$ is related to the wavelength $\lambda$ by $c = \nu\lambda$, so $\nu = c/\lambda$.
$ \frac{hc}{\lambda} = 13.6 \left(\frac{1}{n_f^2} - \frac{1}{n_i^2}\right) \, eV $
Rearranging to find the reciprocal of the wavelength (wavenumber, $1/\lambda$):
$ \frac{1}{\lambda} = \frac{13.6 \, eV}{hc} \left(\frac{1}{n_f^2} - \frac{1}{n_i^2}\right) $
The term $\frac{13.6 \, eV}{hc}$ is a constant. Let's calculate its value: $13.6 \, eV = 13.6 \times (1.602 \times 10^{-19} \, J)$. $h = 6.626 \times 10^{-34} \, J \cdot s$. $c = 3 \times 10^8 \, m/s$. $hc = (6.626 \times 10^{-34} \, J \cdot s) \times (3 \times 10^8 \, m/s) = 1.9878 \times 10^{-25} \, J \cdot m$. $ \frac{13.6 \, eV}{hc} = \frac{13.6 \times 1.602 \times 10^{-19} \, J}{1.9878 \times 10^{-25} \, J \cdot m} \approx \frac{21.787 \times 10^{-19}}{1.9878 \times 10^{-25}} \, m^{-1} $ $ \approx 10.96 \times 10^6 \, m^{-1} = 1.096 \times 10^7 \, m^{-1} $
This constant is the Rydberg constant for hydrogen ($R_H$) that appeared in the empirical Rydberg formula for hydrogen spectrum.
$ \frac{1}{\lambda} = R_H \left(\frac{1}{n_f^2} - \frac{1}{n_i^2}\right) $
This formula, derived from Bohr's model, is identical to the empirical formula, with $n_1 = n_f$ and $n_2 = n_i$. This was a major success for Bohr's theory, as it explained the origin of the spectral lines and calculated the Rydberg constant from fundamental physical constants ($R_H = \frac{m_e e^4}{8\epsilon_0^2 h^3 c}$).
The different spectral series correspond to electron transitions ending in different final energy levels ($n_f$):
- Lyman series: $n_f = 1$, $n_i = 2, 3, 4, ...$ (UV region)
- Balmer series: $n_f = 2$, $n_i = 3, 4, 5, ...$ (Visible region)
- Paschen series: $n_f = 3$, $n_i = 4, 5, 6, ...$ (IR region)
- Brackett series: $n_f = 4$, $n_i = 5, 6, 7, ...$ (IR region)
- Pfund series: $n_f = 5$, $n_i = 6, 7, 8, ...$ (IR region)
Energy level diagram showing transitions for hydrogen spectral series.
Example 1. Calculate the wavelength of the H-beta line in the Balmer series of the hydrogen spectrum. (Rydberg constant $R_H = 1.097 \times 10^7 \, m^{-1}$).
Answer:
Given:
Rydberg constant, $R_H = 1.097 \times 10^7 \, m^{-1}$
For the Balmer series, the final state is $n_f = 2$. The lines in the Balmer series correspond to transitions from $n_i = 3, 4, 5, ...$. The first line (H-alpha) is $n_i=3 \to n_f=2$. The second line (H-beta) is $n_i=4 \to n_f=2$.
We use the Rydberg formula: $ \frac{1}{\lambda} = R_H \left(\frac{1}{n_f^2} - \frac{1}{n_i^2}\right) $
Substitute $n_f = 2$ and $n_i = 4$:
$ \frac{1}{\lambda} = (1.097 \times 10^7 \, m^{-1}) \left(\frac{1}{2^2} - \frac{1}{4^2}\right) $
$ \frac{1}{\lambda} = (1.097 \times 10^7) \left(\frac{1}{4} - \frac{1}{16}\right) \, m^{-1} $
$ \frac{1}{\lambda} = (1.097 \times 10^7) \left(\frac{4 - 1}{16}\right) \, m^{-1} $
$ \frac{1}{\lambda} = (1.097 \times 10^7) \left(\frac{3}{16}\right) \, m^{-1} $
$ \frac{1}{\lambda} = \frac{3.291}{16} \times 10^7 \, m^{-1} \approx 0.20569 \times 10^7 \, m^{-1} $
$ \frac{1}{\lambda} \approx 2.0569 \times 10^6 \, m^{-1} $
Now, find the wavelength $\lambda = 1 / (1/\lambda)$:
$ \lambda = \frac{1}{2.0569 \times 10^6 \, m^{-1}} \approx 0.4862 \times 10^{-6} \, m $
$ \lambda = 4.862 \times 10^{-7} \, m = 486.2 \, nm $
The wavelength of the H-beta line in the Balmer series is approximately 486.2 nm. This is in the blue-green part of the visible spectrum.