Energy is the one observable whose operator also runs the clock. Everything odd about this chapter follows from Δ€ doing two jobs that no other operator does at once.
Chapter 3 handled position and momentum. Chapter 4 does energy β and energy turns out to be different in kind, because its operator is not merely another observable. It is also what drives time forward.
The chapter states its destination in its first paragraph, and it is worth holding onto:
the observable properties of a quantum state with a sharply defined energy never change.
4.1 The Hamiltonian Operator
Β§3.5 established that observables are described by operators and gave two of them:
The energy observable gets an operator too β the Hamiltonian operator hamiltonian operator Δ€ = β(Δ§Β²/2m)βΒ² + V(r). It plays two roles at once: the energy observable, and the generator of time evolution β the SchrΓΆdinger equation is just iΔ§ βΞ¨/βt = Δ€Ξ¨. defined in ch. 4 β open in glossary , written . Phillips builds it by assumption, and says so: the relation between the operators for energy, momentum and position is taken to mirror the relation between the classical quantities. Classically , so
and substituting Eq. (4.1) turns that into something you can actually apply:
The dual role
Here is the observation the whole chapter turns on. does two different jobs.
First, it is the energy observable. The recipe of Β§3.5 β sandwich the operator between and , integrate β gives the energy expectation value directly:
Second, it governs time evolution, because the SchrΓΆdinger equation, Eq. (2.17), is nothing more than
That is the fundamental connection between energy and time, and everything in this chapter is a consequence of it.
How we will solve it
Equation (4.5) is a partial differential equation in four variables. Phillips announces the strategy plainly, and notes it is the same one used for the classical wave equation or the diffusion equation: seek a separable solution, then solve an eigenvalue problem.
Rather than introduce that abstractly, he does something better β he solves a problem you can already picture.
4.2 Normal Modes of a String
Let be the transverse displacement of a stretched string. It obeys the classical wave equation
with the wave speed, and if the ends are fixed at and ,
Separating the variables
The separated equation itself is Eq. (4.9); equating each side to splits it into Eq. (4.10) for the time factor, whose solution is Eq. (4.11), and an equation for the spatial shape:
Where quantization comes from
The general solution of Eq. (4.12) is . Now apply the boundary conditions, and watch what happens:
- kills the cosine, so .
- then requires , so must be a whole multiple of :
can no longer take just any value. There are infinitely many solutions, one per integer:
for , and combining with Eq. (4.11) at gives the complete normal mode:
Figure 4.1 β the four shapes
The general motion, and a change of vocabulary
Because Eq. (4.6) is a homogeneous linear partial differential equation, any superposition of normal modes is also a solution β and in fact the general motion of the string is exactly that:
Given the initial displacement and velocity of every point, ordinary Fourier series techniques find every and .
Phillips then does something quietly clever: he renames what he has just done. No new mathematics, only quantum vocabulary attached to steps you have already taken.
| What we did | What it is called |
|---|---|
| Solved Eq. (4.12) subject to Eq. (4.13) | solved an eigenvalue problem eigenvalue problem A differential equation plus boundary conditions that has solutions only for particular values of a parameter. Discretized, it is exactly the matrix eigenvalue problem you already know. defined in ch. 4 β open in glossary |
| Found solutions exist only for | found the eigenvalues |
| the eigenfunction eigenfunction A function an operator returns unchanged apart from a multiplying constant: Δ€Ο = EΟ. The continuous analogue of an eigenvector, and the constant E is the eigenvalue. defined in ch. 4 β open in glossary belonging to | |
| Wrote the general motion as Eq. (4.16) | expanded in a superposition of eigenfunctions |
What comes next
Everything on this page was classical physics. Not one line of it mentioned , and a vibrating string is as concrete an object as physics has.
Β§4.3 now runs this exact procedure on the SchrΓΆdinger equation β same separation, same eigenvalue problem, same superposition at the end. Only one thing changes: because Eq. (4.5) is first order in time rather than second, the time factor comes out as instead of .
That one difference is the whole chapter.
Check yourself
0 / 7 answered
1.What is meant by the Hamiltonian's "dual role"?
2.In the separation of variables, why must both sides of equal a constant?
3.What actually quantizes for the string?
4.In Fig. 4.1 the eigenfunctions peak at about 1.41 rather than 1. Why?
5.A single normal mode keeps its shape as it vibrates. What does that correspond to mathematically?
6.Discretized, separation of variables turns out to be which linear-algebra operation?
7.The string's frequencies go as , but the box's energies will go as . Where does the difference come from?