← Labs|Radial Probability Distribution — Hydrogen-like Orbitals
Select Orbitals
Atomic Number Z = 1
HKr
r max = 30 a₀
Key Formula
P(r) = r² |R_nl(r)|²
Radial nodes = n − l − 1
Total nodes = n − 1
r_mp ≈ n²a₀/Z (for s)
Total nodes = n − 1
r_mp ≈ n²a₀/Z (for s)
Radial Probability Density P(r) = r² |Rnl|² for Z = 1
1sn=1, l=0, nodes=0
No radial nodes. One smooth peak very close to nucleus. Most penetrating orbital.
Node r: no nodes · Maximum — closest to nucleus
2sn=2, l=0, nodes=1
One radial node creates inner and outer lobe. Inner lobe penetrates — 2s penetrates more than 2p.
Node r: 2.0a₀ · High — inner lobe penetrates
2pn=2, l=1, nodes=0
No radial nodes. Peaks farther from nucleus than 2s. Three degenerate px, py, pz.
Node r: no nodes · Lower than 2s
Penetration Order
ns > np > nd > nf
Why 4s before 3d?
4s penetrates inner shells better than 3d → lower effective Z_eff → lower energy. After 3d fills, 3d drops below 4s.
Anomalies: Cr, Cu
Cr: [Ar]3d⁵4s¹ (not 3d⁴4s²)
Cu: [Ar]3d¹⁰4s¹ (not 3d⁹4s²)
Half-filled/fully-filled d is extra stable.
Slater Rules (σ)
Z_eff = Z − σ
• Same n: 0.35 (0.30 for 1s)
• (n−1): 0.85 for s/p, 1.0 for d/f
• (n−2) and below: 1.0
Higher n_eff = less penetration
Lanthanide Contraction
4f poor penetration → high Z_eff for 4f electrons → small lanthanide radii. 5d ≈ 4d in size due to this.
JEE Focus
• Nodes: n−l−1 radial, l angular
• Degenerate: same n+l (fill order)
• Aufbau: fill lowest n+l first
• Hund: maximize spin in degenerate