From Thomson's model to Bohr's quantized orbits — understanding atomic structure and spectra
By the nineteenth century, enough evidence had accumulated in favour of atomic hypothesis of matter. In 1897, the experiments on electric discharge through gases carried out by J.J. Thomson revealed that atoms of different elements contain negatively charged constituents (electrons) that are identical for all atoms. However, atoms on a whole are electrically neutral. Therefore, an atom must also contain some positive charge to neutralise the negative charge of the electrons.
Thomson proposed the "plum pudding" model: electrons are embedded in a uniformly distributed positive charge sphere, like plums in a pudding. This model could not explain the results of Rutherford's later experiments.
Rutherford's α-particle scattering experiment led to the nuclear model of the atom:
According to classical electrodynamics, an accelerating charge radiates energy. An orbiting electron would lose energy, spiral into the nucleus, and the atom would collapse in ~10⁻¹¹ s. But atoms are stable!
Niels Bohr (1913) postulated a model that explained atomic stability and spectra:
The spectral lines of hydrogen are explained by transitions between energy levels:
n₁ = 1. Ultraviolet region. All lines converge to 91.2 nm limit.
n₁ = 2. Visible region (400-700 nm). First observed series.
n₁ = 3. Infrared region. Lines beyond visible spectrum.
n₁ = 4, 5. Far infrared. Used in astronomical observations.
de Broglie explained Bohr's quantization condition using the wave nature of electrons. An electron in a circular orbit must form a standing wave: