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 () and energies ().
Explains spectral lines via the Rydberg formula (), categorizing transitions into series like Lyman (), Balmer (), etc., which arise from quantized energy differences.
The Schrödinger Equation and Atomic Orbitals
Provides spatial probability densities () for electron positions, reflecting a quantum mechanical view.
Solutions (wavefunctions) are labeled by four quantum numbers:
Principal quantum number (): defines energy and size.
Angular momentum quantum number (): defines orbital shape (s, p, d, f).
Magnetic quantum number (): defines orbital orientation.
Spin quantum number (): describes electron spin.
Wavefunctions separate into radial () and angular () parts: .
Shapes and Radial Probability Distributions
Radial probability density () gives the probability of finding an electron at distance .
Orbitals have nodes (regions of zero probability):
Total nodes:
Radial nodes:
s orbitals () have non-zero density at the nucleus (high penetration), while higher orbitals have nodes near the nucleus.
Increasing 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 are degenerate (have the same energy).
In multi-electron atoms, this degeneracy is lifted by electron-electron interactions, making energy dependent on both and .