3D probability density clouds of hydrogen-like atomic orbitals. The wavefunction ψ(n,l,m) is computed from Laguerre polynomials and spherical harmonics, then visualised via Monte Carlo sampling.
The hydrogen atom's electron is described by ψ(r,θ,φ) — a solution to the Schrödinger equation. It encodes all measurable properties of the electron's state.
|ψ|² gives the probability density — the likelihood of finding the electron at any given point in space. Dense clouds = high probability regions.
n sets the energy level, l determines the orbital shape (s, p, d, f...), and m controls orientation in space.
The radial part R_nl uses associated Laguerre polynomials and determines how ψ varies with distance from the nucleus. Nodes appear where R = 0.