We have seen how Bohr’s postulate accounted for the quantization of energy. Let us now take a look at how Schrödinger’s theory does it.

We begin by observing that if the potential V is independent of time, the Schrödinger equation (2.3.7) has solutions of the form ψ(x,y,z,t) = Ψ(x,y,z)[1:−ωt], where Ψ(x,y,z) is (obviously) independent of time. (You may want to pay attention to the difference between ψ and Ψ.) These solutions are stationary in the sense that the probabilities defined by ψ(x,y,z,t) are independent of time. Inserting such a solution into Eq. (2.3.7) yields the time-independent Schrödinger equation:

(2.5.1) EΨ = −(ℏ^{2}/2m) [(∂_{x})^{2} + (∂_{y})^{2} + (∂_{z})^{2}]Ψ + VΨ.

Returning to one spatial dimension, we cast Eq. (2.5.1) into the following form:

(2.5.2) (∂_{x})^{2}Ψ = AΨ with A = (2m/ℏ^{2})(V − E).

Because Eq. (2.5.2) does not contain any complex numbers (apart from, possibly, Ψ itself), it has real-valued solutions. So let us assume that Ψ is real.

The first thing we notice is that if V is greater than E then Ψ and (∂_{x})^{2}Ψ have the same sign, and if E is greater than V then Ψ and (∂_{x})^{2}Ψ have opposite signs. To see what this means, we need to know a bit more about the operator ∂_{x}. If we plug in the function Ψ(x), out pops another function Ψ’(x):

Ψ’(x) = ∂_{x}Ψ(x).

Its value at any particular place x equals the slope of Ψ(x) at that place, and this equals the slope of the tangent on the graph of Ψ at that place. (The slope of a straight line such as this tangent tells us how steeply it ascends or, if negative, descends from left to right.)

The operator (∂_{x})^{2}Ψ = ∂_{x} (∂_{x}Ψ) = ∂_{x}Ψ’, accordingly, yields the slope of the slope of Ψ. What does this mean? Simply, if the slope of the slope of Ψ is positive, the slope of Ψ increases (from left to right), and the graph of Ψ curves upward as a result. Similarly, if the the slope of the slope of Ψ is negative, the slope of Ψ decreases (from left to right), and the graph of Ψ curves downward as a result.

Thus if Ψ and (∂_{x})^{2}Ψ have the same sign, the graph of Ψ curves upward wherever Ψ is positive (that is, where its graph lies above the x-axis), and it curves downward wherever Ψ is negative (that is, where its graph lies below the x-axis). In either case it bends away from the x-axis. On the other hand, if Ψ and (∂_{x})^{2}Ψ have opposite signs, the graph of Ψ curves downward wherever Ψ is positive, and it curves upward wherever Ψ is negative. In either case it bends toward the x-axis.

So if V is greater than E, the graph of Ψ bends away from the x-axis, and if E is greater than V, the graph of Ψ bends toward the x-axis. In the first case it crosses the x-axis at most once; in the second case it keeps crossing and re-crossing the x-axis exactly like a wave.

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We are now ready to sketch solutions of Eq. (2.5.2) that describe a particle trapped inside a potential well like that in Fig. 2.5.1. Between x_{1} and x_{2}, the particle’s total energy E exceeds the potential energy V, and Ψ exhibits wavelike behavior. To the left of x_{1} and to the right of x_{2}, V exceeds E, and the graph of Ψ bends away from the x-axis. (A classical particle would oscillate back and forth between these two points.)

To obtain a normalized solution (for which the probability of finding the particle anywhere equals unity), we must make sure that the graph of Ψ approaches the x-axis asymptotically in both the limits x→−∞ and x→+∞. Together with the particular form of V(x), these conditions determine both the value and the slope of Ψ at x_{1} and at x_{2}, and these must be exactly matched by the graph of Ψ between these points. For such a match to occur, the value of E must be exactly right. Once again the possible (“allowed”) energies form a sequence E_{n}, starting with n=0, n counting the number of nodes. (Nodes are points at which Ψ crosses the x-axis.)

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Let us remind ourselves in concluding of the sense in which the solutions of Fig. 2.5.2 describe a particle trapped inside a potential well. Like every probability algorithm in quantum mechanics, Ψ serves one and only one purpose: to calculate the probabilities of possible measurement outcomes on the basis of actual outcomes (as well as, generally, some classical boundary conditions). Given the potential V (a classical boundary condition), and given a particle whose energy has been found to equal E_{m}, the probability of finding the particle in the interval I between any two points x=a and x=b (provided that the appropriate measurement is made) is

p(I) = ∫_{(a,b)}dx |Ψ(x)|^{2}.

Here the symbol ∫_{(a,b)}dx indicates a summation over the points contained I: each contributes a complex number |ψ(x)|^{2}. The Fourier transform of Ψ(x), on the other hand, allows us to calculate the probability of finding the particle’s momentum in any given interval of the p– or k-axis.