Allowed energy levels of electrons

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SUMMARY

The quantization of electron energy levels is fundamentally linked to their wave-like behavior and the imposition of boundary conditions in quantum mechanics. When solving the Schrödinger equation for systems like the hydrogen atom, the requirement that the wavefunction remains bounded leads to a discrete set of allowed energy states. This phenomenon is further explained by the concept of standing waves, where certain energy levels correspond to stable configurations that do not cancel out. The values of quantum numbers also play a crucial role in defining these allowed states.

PREREQUISITES
  • Understanding of quantum mechanics principles
  • Familiarity with the Schrödinger equation
  • Knowledge of wave-particle duality
  • Basic concepts of quantum numbers
NEXT STEPS
  • Study the implications of boundary conditions in quantum mechanics
  • Explore the concept of standing waves in quantum systems
  • Learn about the role of quantum numbers in defining electron states
  • Investigate the solutions to the Schrödinger equation for various atomic models
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Students and professionals in physics, particularly those focused on quantum mechanics, atomic theory, and anyone seeking to understand the fundamental principles governing electron behavior in atoms.

Jimmy87
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What is the fundamental reason why the allowed energies of electrons are quantized? I did some research on the web before posting this and what I found seems to link this to the wave-like behaviour of electrons. That is, if electrons could hypothetically exist within the band gaps of the atom, then the electron wave would effectively cancel itself out (like standing waves which effectively give no waves between the various harmonics). Therefore, as it would cancel itself out it cannot exist there. Is this an accepted explanation? I thought that the allowed energy states also depend on the values of the various quantum numbers of the electrons?
 
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When you solve the Schrödinger equation of a quantum system, you initially get a continuous spectrum of states as a solution. However, one has to impose boundary conditions, for example, the electron wavefunction can't grow without bound when one goes arbitrarily far from the nucleus of a hydrogen atom. The boundary conditions restrict the allowed spectrum of electronic states to a discrete (quantized) spectrum.
 

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