Hydrogen Atom
Energy levels, orbitals and spectral transitions
Energy levels of hydrogen-like atoms follow from Bohr quantization. Z is the nuclear charge (H=1, He⁺=2, Li²⁺=3...).
The full wave function separates into radial and angular parts:
Quantum numbers: n=1,2,3... (principal); l=0..n-1 (orbital: s,p,d,f); m=-l..+l (magnetic).
L — associated Laguerre polynomial. a₀=0.0529 nm — Bohr radius.
Electromagnetic transitions are only allowed for specific changes in quantum numbers:
| Series | Lower level | λ (nm) | Region |
|---|---|---|---|
| Lyman | 1 | 91–122 | UV |
| Balmer | 2 | 365–656 | VIS/UV |
| Paschen | 3 | 820–1875 | IR |
| Brackett | 4 | 1458–4051 | IR |
n=1 (1s) — ground state, most stable. n→∞ — ionization (E=0). Number of radial nodes: n-l-1. 1s orbital — Gaussian shape, 2p — node at center.
Q1. What is the ground state energy of the hydrogen atom?
Q2. How many orbitals exist for n=2 (counting l and m)?
Q3. The Balmer series corresponds to transitions to which level?
Q4. He⁺ (Z=2) ground state energy compared to H?