Q4(b). Schrödinger wave equation in three dimensions; meaning of ψ and ψ²
Set up the Schrödinger's wave equation in 3-dimension. Comment on the nature of the equation and various terms involved. Explain the significance of ψ and ψ².
Answer in brief
∂²ψ∂ x²+∂²ψ∂ y²+∂²ψ∂ z²+8π²mh²(E-V)ψ=0, or Hψ=Eψ: a linear, second-order partial differential (eigenvalue) equation. ψ is the amplitude function that describes the state; ψ² dτ is the probability of finding the particle in the volume dτ.
Key points
- A standing wave of amplitude ψ(x,y,z) and wavelength λ obeys the classical wave equation: ∇²ψ+4π²λ²ψ=0, where ∇²=∂²∂ x²+∂²∂ y²+∂²∂ z²
- The particle has a de Broglie wavelength λ=h/mv, so 1λ²=m²v²h².
- Its kinetic energy is total minus potential energy: 12mv²=E-V, so m²v²=2m(E-V).
- ∇²ψ+8π²mh²(E-V)ψ=0 or [-ħ²2m∇²+V]ψ=Eψ, i.e. Hψ=Eψ.
The full model answer
Written out in full, as it should go in the answer booklet. The solution page with its diagrams follows it.
Setting up the equation
- A standing wave of amplitude ψ(x,y,z) and wavelength λ obeys the classical wave equation: ∇²ψ+4π²λ²ψ=0, where ∇²=∂²∂ x²+∂²∂ y²+∂²∂ z²
- The particle has a de Broglie wavelength λ=h/mv, so 1λ²=m²v²h².
- Its kinetic energy is total minus potential energy: 12mv²=E-V, so m²v²=2m(E-V).
- Substituting: ∇²ψ+8π²mh²(E-V)ψ=0 or [-ħ²2m∇²+V]ψ=Eψ, i.e. Hψ=Eψ.
Nature of the equation and its terms
- It is a second-order, linear, homogeneous partial differential equation in x, y, z; it is time-independent (stationary states). Any multiple or sum of solutions of equal E is also a solution.
- It is an eigenvalue equation: H (the Hamiltonian, energy operator) acting on ψ returns a number, E, times ψ. Acceptable solutions exist only for certain values of E: quantisation follows from the boundary conditions, not from an extra assumption.
- Terms: m mass of the particle; E total energy (eigenvalue); V(x,y,z) potential energy (for the H atom -e²/4πε₀r); h Planck's constant; -ħ²2m∇² the kinetic-energy operator; ψ the wave function (eigenfunction).
Significance of ψ and ψ²
- ψ is the amplitude of the matter wave and contains all that can be known about the state. It has no direct physical meaning: it can be negative (as beyond the node of the 2s orbital, panel) or complex. Its sign matters in overlap and bonding.
- An acceptable ψ must be single-valued, continuous, finite and have a continuous first derivative; it must vanish at infinity so that it can be normalised.
- Born interpretation: ψ² (strictly ψ*ψ=|ψ|²) is the probability density; ψ² dτ is the probability of finding the particle in the volume element dτ. It is never negative.
- Normalisation: ∫ψ² dτ=1 over all space (the particle is somewhere). Where ψ=0 (a node) the particle is never found; regions of large ψ² define the shape of an orbital.
Application. the same equation with the Coulomb potential gives the hydrogen orbitals, the quantum numbers n, l, mₗ and the energies Eₙ=-13.6/n² eV; with V=0 inside a box it gives the particle-in-a-box levels used for conjugated dyes.
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All parts of Question 4
- 4(a)(i) Stark–Einstein law; quantum yield and why it is often low15 marks
- 4(a)(ii) Principle of polarography; the half-wave potential10 marks
- 4(b) Schrödinger wave equation in three dimensions; meaning of ψ and ψ²15 marks
- 4(c) Equilibrium constant of A + B ⇌ C from two relaxation times10 marks