Atomic Structure and Spectra

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Course Outline

  1. Bohr's quantization condition
  2. Allowed stationary orbits
  3. Energy absorption and emission
  4. Hydrogen atom model
  5. Energy levels and spectra
  6. Hydrogen-like atoms
  7. Excitation and ionization energies
  8. Limitations of Bohr's theory

1. Bohr's quantization condition

Key Concepts & Definitions

Bohr's quantization condition:
BOHR (1913): The principle that the angular momentum of an electron in an atom is restricted to discrete, quantized values. Specifically, the angular momentum can only take on values that are integer multiples of ħ, where ħ is the reduced Planck constant. This is expressed mathematically as mvr=nm v r = n \hbar, where mm is the mass of the electron, vv is its velocity, rr is the radius of the orbit, and nn is a positive integer called the principal quantum number.

Angular momentum quantization:
The concept that the angular momentum of an electron orbiting the nucleus is not continuous but can only have specific, discrete values. These values are integral multiples of \hbar, meaning the electron's angular momentum is quantized.

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Anteprima del quiz

1. How is Bohr's quantization condition applied to determine the properties of an electron's orbit in practice?

2. What is the key property that defines allowed stationary orbits in Bohr's model of the atom?

3. What does energy absorption and emission fundamentally mean in atomic transitions?

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Anteprima delle flashcard

Bohr's quantization condition

Electron angular momentum is quantized as discrete values.

Allowed stationary orbits

Electrons in stable, non-radiating orbits with quantized radii and velocities.

Energy absorption — process?

Electron absorbs photon energy to move to a higher energy level.

Energy emission — process?

Electron releases photon energy when transitioning to a lower level.

Hydrogen atom model

Electron orbits nucleus in quantized circular paths with negative total energy.

Energy levels — formula?

En = -13.6 eV / n², with n as quantum number.

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