[This problem generalizes Example 1.2.] Imagine a particle of mass m and energy E in a potential well V(X), sliding frictionlessly back and forth between the classical turning points (a and b in Figure 1.10). Classically, the probability of finding the particle in the range dx (if, for example, you took a snapshot at a random time t) is equal to the fraction of the time T it takes to get from a to b that it spends in the interval dx:
ρ(x) d x=\frac{d t}{T}=\frac{(d t / d x) d x}{T}=\frac{1}{v(x) T} d x (1.41)
where v(x) is the speed, and
T=\int_{0}^{T} d t=\int_{a}^{b} \frac{1}{v(x)} d x . (1.42).
Thus
ρ(x) = \frac{1}{v(x)T} (1.43).
This is perhaps the closest classical analog to \left|\Psi \right|^2 .
(a) Use conservation of energy to express v(x) in terms of E and V(x) .
(b) As an example, find ρ(x) for the simple harmonic oscillator, V(x) = kx^2/2 . Plot ρ(x), and check that it is correctly normalized.
(c) For the classical harmonic oscillator in part (b), find \left\langle x\right\rangle ,\left\langle x^2\right\rangle and σ_x .