Orbital Presets
Wave Function Equations
Rnl(r) = 2 · e-r
Ylm(θ,φ) = 1/√(4π)
Explore the quantum mechanical probability distribution of hydrogen electron clouds
The hydrogen atom wave function describes the quantum mechanical behavior of electrons in a hydrogen atom. Unlike classical physics, electrons do not move in fixed orbits but exist as probability clouds around the nucleus. The square of the wave function |ψ|² gives the probability density of finding an electron at a given point in space.
Range: n = 1, 2, 3, 4, ...
Physical Meaning: Determines the electron's energy level (shell). Larger n means higher energy and greater average distance from the nucleus. Bohr radius a₀ ≈ 0.529 Å is the natural length unit.
Range: l = 0, 1, 2, ..., n-1
Physical Meaning: Determines orbital angular momentum magnitude and shape.
l=0: s orbitals (spherical)
l=1: p orbitals (dumbbell)
l=2: d orbitals (cloverleaf)
l=3: f orbitals (complex multi-lobed)
Range: m = -l, -l+1, ..., 0, ..., l-1, l
Physical Meaning: Determines spatial orientation of the orbital. In external magnetic fields, orbitals with different m values have slightly different energies (Zeeman effect).
-ħ²/(2m) ∇²ψ - e²/(4πε₀r)ψ = Eψ
ψnlm(r,θ,φ) = Rnl(r) · Ylm(θ,φ)
Rnl(r) = √[(2/n a₀)³ (n-l-1)!/(2n[(n+l)!])] · (2r/n a₀)l · Ln-l-12l+1(2r/n a₀) · e-r/n a₀
Ylm(θ,φ) = √[(2l+1)/(4π) · (l-|m|)!/(l+|m|)!] · Pl|m|(cosθ) · eimφ
P(r,θ,φ) = |ψnlm(r,θ,φ)|² = |Rnl(r)|² · |Ylm(θ,φ)|²
Nodal surfaces are surfaces where the wave function equals zero, divided into two types:
Spherically symmetric, no nodes, maximum probability density at the nucleus. The ground state (lowest energy) of hydrogen.
Spherically symmetric with one spherical radial node (at r=2a₀). Probability distribution extends further than 1s.
Dumbbell-shaped with one angular nodal plane through the nucleus. Three degenerate 2p orbitals oriented along x, y, z axes.
Cloverleaf-shaped with two angular nodal surfaces. Five 3d orbitals have different spatial orientations.
In 1913, Niels Bohr proposed the Bohr model, introducing quantization to atomic structure. In 1926, Erwin Schrödinger established the wave equation, providing a complete quantum mechanical description of atomic structure. Also in 1926, Wolfgang Pauli proposed the exclusion principle, explaining electron arrangement rules. Together, these works laid the foundation of quantum mechanics, revolutionizing our understanding of the microscopic world.