Hydrogen-like Atomic Orbitals and Schrödinger Equation – Exam Prep Notes

The Bohr Model of Hydrogen
  • Treats hydrogen with electrons in stationary orbits with quantized radii (r<em>n=a</em>0n2r<em>n = a</em>0 n^2) and energies (En=13.6 eVn2E_n = - \frac{13.6\ \text{eV}}{n^2}).

  • Explains spectral lines via the Rydberg formula (1λ=R<em>H(1n</em>121n<em>22)\frac{1}{\lambda} = R<em>H\left( \frac{1}{n</em>1^2} - \frac{1}{n<em>2^2} \right)), categorizing transitions into series like Lyman (n</em>1=1n</em>1 = 1), Balmer (n1=2n_1 = 2), etc., which arise from quantized energy differences.

The Schrödinger Equation and Atomic Orbitals
  • Provides spatial probability densities (ψ(r,θ,ϕ)2|\psi(r,\theta,\phi)|^2) for electron positions, reflecting a quantum mechanical view.

  • Solutions (wavefunctions) are labeled by four quantum numbers:

    1. Principal quantum number (nn): 1,2,3,,1,2,3,\dots, defines energy and size.

    2. Angular momentum quantum number (ll): 0,1,2,,(n1),0,1,2,\dots,(n-1), defines orbital shape (s, p, d, f).

    3. Magnetic quantum number (mm): l,,l,-l,\dots,l, defines orbital orientation.

    4. Spin quantum number (msm_s): +12,12,+\frac{1}{2}, -\frac{1}{2}, describes electron spin.

  • Wavefunctions separate into radial (R<em>n,l(r)R<em>{n,l}(r)) and angular (Y</em>lm(θ,ϕ)Y</em>l^m(\theta,\phi)) parts: ψ<em>n,l,m(r,θ,ϕ)=R</em>n,l(r)Ylm(θ,ϕ)\psi<em>{n,l,m}(r,\theta,\phi) = R</em>{n,l}(r)\,Y_l^m(\theta,\phi).

Shapes and Radial Probability Distributions
  • Radial probability density (P<em>radial(r)=4πr2R</em>n,l(r)2Ylm(θ,ϕ)2P<em>{\text{radial}}(r) = 4\pi r^2 |R</em>{n,l}(r)|^2 |Y_l^m(\theta,\phi)|^2) gives the probability of finding an electron at distance rr.

  • Orbitals have nodes (regions of zero probability):

    • Total nodes: n1n-1

    • Radial nodes: nl1n-l-1

  • s orbitals (l=0l=0) have non-zero density at the nucleus (high penetration), while higher ll orbitals have nodes near the nucleus.

  • Increasing nn for a given orbital type makes the orbital larger and increases the number of radial nodes.

The Hydrogenic Orbitals and Energy Degeneracy
  • In a pure hydrogen-like atom, all orbitals with the same nn are degenerate (have the same energy).

  • In multi-electron atoms, this degeneracy is lifted by electron-electron interactions, making energy dependent on both nn and ll.