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Bohr’s Model of the Hydrogen Atom


1. Introduction

Classical physics failed to explain the stability of atoms and the discrete nature of atomic spectra.
Rutherford’s nuclear model predicted that orbiting electrons should continuously radiate energy and spiral into the nucleus. To resolve these contradictions, Niels Bohr (1913) proposed a quantum model for the hydrogen atom.


2. Experimental Motivation


3. Bohr’s Postulates

(i) Stationary Orbits

Electrons revolve around the nucleus only in certain allowed circular orbits without radiating energy.

(ii) Quantization of Angular Momentum

The angular momentum of the electron is quantized:

\[mvr = n\hbar, \quad n = 1,2,3,\dots\]

(iii) Emission and Absorption of Radiation

Radiation is emitted or absorbed only during transitions between allowed orbits:

\[h\nu = E_i - E_f\]

4. Force Balance in the Atom

For an electron in a circular orbit, the electrostatic force provides the centripetal force:

\[\frac{1}{4\pi\varepsilon_0}\frac{e^2}{r^2} = \frac{mv^2}{r}\]

5. Radius of Allowed Orbits

Using force balance and angular momentum quantization, the radius of the $n^{\text{th}}$ orbit is:

\[\boxed{ r_n = \frac{4\pi\varepsilon_0 \hbar^2}{m e^2} \, n^2 }\]

The smallest allowed radius (Bohr radius):

\[\boxed{ a_0 = 0.529 \, \text{Å} }\]

Hence,

\[\boxed{ r_n = n^2 a_0 }\]

6. Velocity of the Electron

The velocity of the electron in the $n^{\text{th}}$ orbit is:

\[\boxed{ v_n = \frac{e^2}{2\varepsilon_0 h} \frac{1}{n} }\]

For the ground state ($n=1$):

\[v_1 \approx 2.18 \times 10^6 \, \text{m s}^{-1}\]

7. Energy of the Electron

Kinetic Energy

\(K = \frac{1}{2}mv^2\)

Potential Energy

\(U = -\frac{1}{4\pi\varepsilon_0}\frac{e^2}{r}\)

Total Energy

\(E = K + U = -\frac{1}{8\pi\varepsilon_0}\frac{e^2}{r}\)

Substituting $r_n$:

\[\boxed{ E_n = -\frac{m e^4}{8 \varepsilon_0^2 h^2} \frac{1}{n^2} }\]

Numerically,

\[\boxed{ E_n = -\frac{13.6}{n^2} \, \text{eV} }\]

8. Hydrogen Spectrum

For a transition from $n_i$ to $n_f$:

\[h\nu = E_{n_i} - E_{n_f}\]

Thus,

\[\boxed{ \nu = \frac{13.6\,\text{eV}}{h} \left(\frac{1}{n_f^2} - \frac{1}{n_i^2}\right) }\]

Rydberg Formula

\[\boxed{ \frac{1}{\lambda} = R \left(\frac{1}{n_f^2} - \frac{1}{n_i^2}\right) }\]

where

\[R = 1.097 \times 10^7 \, \text{m}^{-1}\]

9. Ionization Energy of Hydrogen

Ionization corresponds to $n=1 \rightarrow n=\infty$:

\[\boxed{ E_{\text{ion}} = 13.6 \, \text{eV} }\]

10. Successes of Bohr’s Model


11. Limitations of Bohr’s Model


12. Bohr Model and Quantum Mechanics