Summary
This section traces the evolution of atomic models from early classical ideas to the modern quantum mechanical understanding. Starting with the Bohr model and its quantized orbits, students learn how specific energy levels relate to photon emission and absorption. The introduction of quantum numbers (n, l, m?, and m?) through experiments such as the Zeeman effect and the Davisson-Germer experiment provides deeper insight into electron configurations and the structure of the periodic table. The sections on de Broglie waves, the uncertainty principle, and quantum tunneling underscore the wave–particle duality that governs microscopic systems, leading to practical applications such as lasers.