Section 4 Flashcards
The time evolution of a quantum state of definite energy is
Ψ(t) = exp[-iEt/ℏ] Ψ(0)
Unitary evolution
|Ψ(t)|^2 = |Ψ(0)|^2 : a stationary state
The eigenvectors of stationary states are also
time-invariant
Time-dependent state evolution
iℏ ∂Ψ(r,t)/∂t = H(hat)Ψ(r,t)
eigenstate of the Hamiltonian
A stationary state has definite energy
The Hamiltonian governs
the time-evolution of the state, and hence the expectation values
Ehrenfest’s Theorem
is an example of the correspondence principle: QM limits to classical physics for large systems
Newtonian momentum derivation
[x(hat),H(hat)] = [x(hat),p(hat)^2/2m + V(x)]
since x(hat) commutes with V(x(hat))
d<x>/dt = 1/2iℏm <[x(hat),p(hat)^2]></x>
=> <p> = m d<r>/dt</r>
similarly derivation gives, [p(hat),H(hat)] =>
d<p>/dt = -<ΔV></ΔV>
Stationary states are
super-important solutions of time-invarient probability density; time-evolution
eigenvalue equation
H(hat) Ψi(x) = EiΨi(x)
The time-independent schrodinger equation
[ -ℏ^2/2m d^2/dx^2 + V(x) ]Ψ(x) = EΨ(x)
Probability conservation
dPtot(t)/dt = 0
Schrodinger equation links
wave-function time evolution and spatial curvature
The flux is a probability current
J(r,t) = ℏ/2im [Ψ∇Ψ - Ψ∇Ψ]