Bohr Model of the Atom

Bohr Model of the Hydrogen Atom
  • Rutherford's Atomic Paradox: Classical physics predicted electrons orbiting a positive nucleus would continuously emit electromagnetic radiation and spiral into the nucleus.

  • Bohr's Postulates (1913):

    • Electrons orbit the nucleus only in specific circular orbits with specific, allowed energies.

    • The hydrogen atom does not emit energy while the electron is in one of these fixed orbits.

    • An electron moves to a different orbit only by emitting or absorbing a photon with energy equal to the difference in energy between the two orbits.

Electron Energies in Hydrogen
  • Energy Equation: The energies of electron orbits in hydrogen are given by:

    • E_n = -\frac{k}{n^2}

    • Where k = 2.18 \times 10^{-18} \text{ J} is a constant, and n is the principal quantum number (orbit number).

  • Significance of Negative Energy: The negative sign indicates that the electron's zero energy point is when it is completely removed from the nucleus (n \to \infty).

  • Energy Levels: More negative energy means lower energy. The n=1 orbit has the lowest energy (ground state). As n increases, the electron's energy and distance from the nucleus increase.

Electron Transitions and Energy Changes
  • Ground State: The lowest energy level, typically where the electron resides (n=1).

  • Excited State: A higher energy level reached when the atom absorbs energy and the electron moves to a higher n orbit.

  • Energy Change for Transitions: The energy change for an electron transition is:

    • \Delta E = -k \left( \frac{1}{n{\text{final}}^2} - \frac{1}{n{\text{initial}}^2} \right)

    • When energy is absorbed (n{\text{initial}} < n{\text{final}}), \Delta E is positive.

    • When energy is emitted (n{\text{initial}} > n{\text{final}}), \Delta E is negative (e.g., electron moves from excited state back to ground state).

  • Photon Properties: The energy of the corresponding photon is equal to the magnitude of \Delta E (E_{\text{photon}} = |\Delta E|).

    • Photon frequency (\nu) and wavelength (\lambda) can be calculated using E_{\text{photon}} = h\nu and \lambda\nu = c.