⚛️ Physics — Class XII

Atoms

From Thomson's model to Bohr's quantized orbits — understanding atomic structure and spectra

📖 Chapter 12 ⏱ ~45 min read 🏷️ Modern Physics

Table of Contents

  1. Introduction
  2. Thomson's Model
  3. Rutherford's Nuclear Model
  4. Bohr's Model of Hydrogen
  5. Hydrogen Spectrum
  6. de Broglie's Explanation

12.1 Introduction

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.

12.2 Thomson's Model

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.

12.3 Rutherford's Nuclear Model

Atoms
Figure 12.1 — Bohr model of hydrogen, spectral series, and atomic models comparison

Rutherford's α-particle scattering experiment led to the nuclear model of the atom:

⚠️ Problem with Rutherford Model

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!

12.4 Bohr's Model of Hydrogen

Niels Bohr (1913) postulated a model that explained atomic stability and spectra:

rₙ = n²a₀/Z | Eₙ = −13.6Z²/n² eV
a₀ = 0.529 Å (Bohr radius). For hydrogen (Z=1): E₁ = −13.6 eV, r₁ = 0.529 Å.

12.5 Hydrogen Spectrum

The spectral lines of hydrogen are explained by transitions between energy levels:

1/λ = R_H(1/n₁² − 1/n₂²)
R_H = 1.097 × 10⁷ m⁻¹ (Rydberg constant). n₁ = lower level, n₂ = upper level.
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Lyman Series

n₁ = 1. Ultraviolet region. All lines converge to 91.2 nm limit.

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Balmer Series

n₁ = 2. Visible region (400-700 nm). First observed series.

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Paschen Series

n₁ = 3. Infrared region. Lines beyond visible spectrum.

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Brackett & Pfund

n₁ = 4, 5. Far infrared. Used in astronomical observations.

12.6 de Broglie's Explanation

de Broglie explained Bohr's quantization condition using the wave nature of electrons. An electron in a circular orbit must form a standing wave:

2πr = nλ = nh/(mv)
This gives L = mvr = nℏ — Bohr's quantization condition emerges naturally from wave mechanics!
Ch 11 — Dual Nature of Radiation Ch 13 — Nuclei