CBSE · Class 12 · Physics · AtomsDiscuss the limitations of Rutherford's atomic model. Explain how Bohr's atomic model successfully overcame these limitations and accounted for the stability of atoms and atomic spectra.
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Limitations of Rutherford's Atomic Model\nAlthough Rutherford's $\alpha$-particle scattering experiment successfully established the nuclear model of the atom (proposing a heavy, positively charged nucleus surrounded by orbiting electrons), it suffered from major theoretical flaws:
- Inability to Explain Stability of Atom: According to classical electrodynamics (Maxwell's theory), any accelerated charged particle must continuously radiate electromagnetic energy. Since an electron revolving in a circular orbit experiences centripetal acceleration, it should continuously lose energy and spiral into the nucleus within a fraction of a second ($~10^{-8}$ s). However, atoms are stable.
- Inability to Explain Line Spectra: According to Rutherford's model, electrons can revolve in any arbitrary orbit. Consequently, they should radiate a continuous spectrum of all frequencies. However, experiments with atomic gases show distinct line spectra (discrete frequencies).
How Bohr's Model Overcame These Limitations\nNiels Bohr in 1913 proposed a new model that successfully resolved the shortcomings of Rutherford's model by introducing quantum postulates:
- Resolution of Stability: Bohr postulated that electrons do not radiate energy while revolving in certain specific non-radiating orbits called stationary orbits. Energy is only emitted or absorbed when an electron jumps between these fixed energy states.
- Resolution of Line Spectra: Since the permitted orbits have fixed, discrete energies ($E_n$), the energy difference $\Delta E = E_2 - E_1$ is also fixed. When an electron transitions from a higher orbit to a lower orbit, a photon of a specific, single frequency ($\nu = \Delta E / h$) is emitted, resulting in discrete line spectra rather than a continuous spectrum. \nThus, Bohr's model successfully bridged classical mechanics and early quantum theory to explain atomic stability and spectral series.
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