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Physics · Quantum Mechanics and Modern Physics

Postulates of Quantum Mechanics, Wave Functions and the Born Interpretation

A particle is described by a complex wave function Ψ(x,t)\Psi(x,t) whose modulus squared ∣Ψ∣2|\Psi|^2 is the position probability density (Born). Ψ\Psi is normalised, ∫∣Ψ∣2 dx=1\int|\Psi|^2\,dx=1, and normalisation is preserved by the continuity equation ∂tρ+∂xj=0\partial_t\rho+\partial_x j=0. Observables are Hermitian operators (x^=x\hat x=x, p^=−iℏ∂x\hat p=-i\hbar\partial_x) with ⟨Q⟩=∫Ψ∗Q^Ψ dx\langle Q\rangle=\int\Psi^*\hat Q\Psi\,dx; a measurement returns an eigenvalue qnq_n with probability ∣cn∣2|c_n|^2 and collapses the state to ψn\psi_n.

Postulates of Quantum Mechanics, Wave Functions and the Born Interpretation

The previous chapter ended with de Broglie's claim that a particle has a wave. This chapter turns that claim into a working framework: a particle is described by a complex wave function Ψ(x,t)\Psi(x,t), its modulus squared is a probability density, and every physical prediction is a statistical statement extracted from Ψ\Psi by a fixed set of rules. Nothing here is derived from classical mechanics; the postulates are justified only by the fact that everything built on them agrees with experiment. We work in one dimension throughout, which contains every conceptual point without the bookkeeping of three.

The organising idea is the statistical interpretation, due to Born. Quantum mechanics does not predict where a particle is; it predicts the probability of each possible outcome of a measurement. Between measurements the state evolves smoothly and deterministically (by the Schrödinger equation, Chapter 3); a measurement is a separate kind of process that returns one eigenvalue at random, with probabilities set by Ψ\Psi, and leaves the system in the corresponding eigenstate. This chapter states the postulates, defines normalisation and probability current, and shows how expectation values and the momentum operator follow.

How to read this chapter. The three things to carry forward are: (i) ∣Ψ∣2|\Psi|^2 is a probability density, so Ψ\Psi must be normalised and normalisation must be preserved in time; (ii) observables are represented by operators, and ⟨Q⟩=∫Ψ∗Q^ Ψ dx\langle Q\rangle = \int \Psi^* \hat Q\,\Psi\,dx; (iii) the momentum operator is p^=−iℏ ∂/∂x\hat p = -i\hbar\,\partial/\partial x, which is what makes [x^,p^]=iℏ[\hat x,\hat p]=i\hbar (Chapter 5) and the uncertainty principle unavoidable.

1. The Wave Function and the Born Rule

Postulate 1 (state). The state of a particle at time tt is a complex-valued function Ψ(x,t)\Psi(x,t), square-integrable over all space.

Postulate 2 (Born rule). If the position of the particle is measured at time tt, the probability of finding it between xx and x+dxx+dx is

P(x,t) dx=∣Ψ(x,t)∣2 dx=Ψ∗(x,t) Ψ(x,t) dxP(x,t)\,dx = |\Psi(x,t)|^2\,dx = \Psi^*(x,t)\,\Psi(x,t)\,dx

The quantity ρ(x,t)=∣Ψ∣2\rho(x,t) = |\Psi|^2 is the position probability density. Only ∣Ψ∣2|\Psi|^2 has direct physical meaning; Ψ\Psi itself is a probability amplitude, and an overall constant phase eiαe^{i\alpha} multiplying Ψ\Psi changes no prediction. Amplitudes, not probabilities, are what superpose — this is the origin of interference.

Born's rule replaces the classical idea of a definite trajectory. Before the measurement the particle does not have a position that Ψ\Psi merely fails to reveal; the indefiniteness is a property of the state, not of our knowledge. This is the orthodox (Copenhagen) position; experiments rule out local hidden-variable alternatives, though other interpretations reproduce the same predictions.

2. Normalisation and Its Preservation

For ∣Ψ∣2|\Psi|^2 to be a probability density it must integrate to one:

∫−∞∞∣Ψ(x,t)∣2 dx=1\int_{-\infty}^{\infty} |\Psi(x,t)|^2\,dx = 1

A solution of the Schrödinger equation can always be scaled to satisfy this, provided the integral is finite (the function is square-integrable, Ψ∈L2\Psi \in L^2). Functions that are not normalisable — a pure plane wave eikxe^{ikx}, for instance — are not physical states on their own, though they are useful building blocks.

Normalisation is preserved in time. If Ψ\Psi is normalised at t=0t=0, it stays normalised. Using the Schrödinger equation one shows

ddt∫−∞∞∣Ψ∣2 dx=[iℏ2m(Ψ∗∂Ψ∂x−Ψ∂Ψ∗∂x)]−∞∞=0\frac{d}{dt}\int_{-\infty}^{\infty} |\Psi|^2\,dx = \left[\frac{i\hbar}{2m}\left(\Psi^*\frac{\partial\Psi}{\partial x} - \Psi\frac{\partial\Psi^*}{\partial x}\right)\right]_{-\infty}^{\infty} = 0

because a normalisable Ψ\Psi and its derivative vanish at infinity. If the equation did not have this property it could not support a probability interpretation at all — so this is a consistency check on the dynamics, not an extra assumption.

3. The Probability Current and the Continuity Equation

Define the probability current

j(x,t)=iℏ2m(Ψ ∂Ψ∗∂x−Ψ∗ ∂Ψ∂x)=ℏm Im ⁣(Ψ∗∂Ψ∂x)j(x,t) = \frac{i\hbar}{2m}\left(\Psi\,\frac{\partial\Psi^*}{\partial x} - \Psi^*\,\frac{\partial\Psi}{\partial x}\right) = \frac{\hbar}{m}\,\mathrm{Im}\!\left(\Psi^*\frac{\partial\Psi}{\partial x}\right)

Then probability obeys a local conservation law, exactly like charge in electrodynamics:

∂ρ∂t+∂j∂x=0\frac{\partial\rho}{\partial t} + \frac{\partial j}{\partial x} = 0

Integrating over a finite interval [a,b][a,b] gives ddt∫abρ dx=j(a,t)−j(b,t)\dfrac{d}{dt}\displaystyle\int_a^b \rho\,dx = j(a,t) - j(b,t): the probability in a region changes only by flowing across its boundaries. Probability is not created or destroyed, only transported. For a stationary state jj is independent of xx; for a real Ψ\Psi (bound states can be chosen real) j=0j = 0 everywhere — the particle is "standing still" in the probabilistic sense.

4. Operators and Expectation Values

Postulate 3 (observables). Every measurable quantity Q(x,p)Q(x,p) is represented by a linear Hermitian operator Q^\hat Q, obtained from the classical expression by the substitutions

x⟶x^=x (multiplication),p⟶p^=−iℏ ∂∂xx \longrightarrow \hat x = x\ (\text{multiplication}),\qquad p \longrightarrow \hat p = -i\hbar\,\frac{\partial}{\partial x}

Postulate 4 (expectation value). The mean of many measurements of QQ on identically prepared systems in state Ψ\Psi is

⟨Q⟩=∫−∞∞Ψ∗(x,t) Q^ Ψ(x,t) dx\langle Q\rangle = \int_{-\infty}^{\infty} \Psi^*(x,t)\,\hat Q\,\Psi(x,t)\,dx

For position this reduces to the obvious ⟨x⟩=∫x ∣Ψ∣2 dx\langle x\rangle = \int x\,|\Psi|^2\,dx. For momentum it gives ⟨p⟩=∫Ψ∗(−iℏ ∂x)Ψ dx\langle p\rangle = \int \Psi^*(-i\hbar\,\partial_x)\Psi\,dx, which is not an average of any pre-existing values — there is no "momentum at xx". The operator ordering matters: xp^\widehat{xp} is ambiguous classically, and the correct quantum operator for such products is the symmetrised (Hermitian) form 12(x^p^+p^x^)\tfrac12(\hat x\hat p + \hat p\hat x).

Worked example — expectation values in the ground state of a box. For Ψ(x)=2/a sin⁡(πx/a)\Psi(x) = \sqrt{2/a}\,\sin(\pi x/a) on [0,a][0,a]: by symmetry ⟨x⟩=a/2\langle x\rangle = a/2; a short integration gives ⟨x2⟩=a2(13−12π2)\langle x^2\rangle = a^2\left(\tfrac13 - \tfrac{1}{2\pi^2}\right); and ⟨p⟩=0\langle p\rangle = 0 (real Ψ\Psi), while ⟨p2⟩=(πℏ/a)2\langle p^2\rangle = (\pi\hbar/a)^2, consistent with E=⟨p2⟩/2m=π2ℏ2/2ma2E = \langle p^2\rangle/2m = \pi^2\hbar^2/2ma^2.

5. Why the Momentum Operator Is −iℏ ∂x-i\hbar\,\partial_x

The form of p^\hat p is fixed by requiring d⟨x⟩dt=⟨p⟩m\dfrac{d\langle x\rangle}{dt} = \dfrac{\langle p\rangle}{m}, the quantum echo of v=p/mv = p/m. Differentiating ⟨x⟩=∫x∣Ψ∣2 dx\langle x\rangle = \int x|\Psi|^2\,dx and using the Schrödinger equation to replace ∂tΨ\partial_t\Psi:

d⟨x⟩dt=∫x ∂ρ∂t dx=−∫x ∂j∂x dx=∫j dx=1m∫Ψ∗(−iℏ ∂x)Ψ dx\frac{d\langle x\rangle}{dt} = \int x\,\frac{\partial\rho}{\partial t}\,dx = -\int x\,\frac{\partial j}{\partial x}\,dx = \int j\,dx = \frac{1}{m}\int \Psi^*(-i\hbar\,\partial_x)\Psi\,dx

(the third step is integration by parts). The last integral is what we must call ⟨p⟩/m\langle p\rangle/m, which identifies p^=−iℏ ∂x\hat p = -i\hbar\,\partial_x. Momentum eigenfunctions are then eipx/ℏe^{ipx/\hbar}: p^ eipx/ℏ=p eipx/ℏ\hat p\,e^{ipx/\hbar} = p\,e^{ipx/\hbar}. Expanding a state in these is the Fourier transform, and ∣Ψ~(p)∣2|\tilde\Psi(p)|^2 is the probability density in momentum space.

6. Superposition and Measurement

Postulate 5 (superposition). If Ψ1\Psi_1 and Ψ2\Psi_2 are possible states, so is any linear combination c1Ψ1+c2Ψ2c_1\Psi_1 + c_2\Psi_2. The space of states is a complex vector space (a Hilbert space, Chapter 4).

Postulate 6 (measurement / collapse). A measurement of an observable Q^\hat Q yields one of its eigenvalues qnq_n. If Ψ=∑ncnψn\Psi = \sum_n c_n \psi_n with Q^ψn=qnψn\hat Q\psi_n = q_n\psi_n and the ψn\psi_n orthonormal, then

Prob(qn)=∣cn∣2,cn=∫ψn∗ Ψ dx\mathrm{Prob}(q_n) = |c_n|^2, \qquad c_n = \int \psi_n^*\,\Psi\,dx

and immediately after the measurement the state is ψn\psi_n (collapse). Between measurements the evolution is the smooth, unitary Schrödinger flow; the collapse is the discontinuous, probabilistic part. The two together are the full dynamics of the orthodox theory. Note ∑n∣cn∣2=1\sum_n |c_n|^2 = 1 is exactly normalisation expressed in the {ψn}\{\psi_n\} basis (Parseval's theorem).

Worked example — a two-state superposition. Let Ψ=15ψ1+25ψ2\Psi = \tfrac{1}{\sqrt5}\psi_1 + \tfrac{2}{\sqrt5}\psi_2 with energies E1,E2E_1,E_2. An energy measurement gives E1E_1 with probability 1/51/5 and E2E_2 with probability 4/54/5; the mean is ⟨H⟩=15E1+45E2\langle H\rangle = \tfrac15 E_1 + \tfrac45 E_2. After a result of E2E_2, an immediate repeat measurement gives E2E_2 with certainty — the state has collapsed to ψ2\psi_2.

7. Admissibility Conditions on Ψ\Psi

For Ψ\Psi to represent a physical state and for the operators above to act sensibly:

  1. Ψ\Psi is single-valued — one amplitude per point.
  2. Ψ\Psi is square-integrable — ∫∣Ψ∣2<∞\int|\Psi|^2 < \infty, so it can be normalised.
  3. Ψ\Psi is continuous, and ∂xΨ\partial_x\Psi is continuous except where the potential has an infinite jump (an infinite wall, or a δ\delta-function, where ∂xΨ\partial_x\Psi may step).
  4. Ψ→0\Psi \to 0 as ∣x∣→∞|x|\to\infty fast enough for (2); its derivative too.

These are not extra postulates but the minimal regularity that makes the probability interpretation and the Schrödinger equation consistent. A "wave function" violating them (e.g. 1/x1/x near the origin, or a step discontinuity in a smooth potential) is unphysical.

8. What the Formalism Does Not Say

  • It does not give trajectories. ⟨x⟩(t)\langle x\rangle(t) moves smoothly (Ehrenfest, Chapter 5), but individual runs give scattered results.
  • It does not explain why a particular outcome occurs on a particular run — only the probabilities. This is the measurement problem, still debated; the orthodox theory simply posits collapse.
  • It is not a hidden-variable theory in disguise: Bell's theorem (beyond this course) rules out local hidden variables reproducing all quantum predictions.
  • ∣Ψ∣2|\Psi|^2 is a probability density in configuration space, not a physical matter density; the electron does not smear out into a charge cloud, though time-averaged it can be treated as one for some purposes.

9. Common Pitfalls

  • Treating Ψ\Psi as observable. Only ∣Ψ∣2|\Psi|^2 (and relative phases in superpositions) are physical; a global phase is irrelevant.
  • Forgetting to normalise before computing probabilities. ∣cn∣2|c_n|^2 are probabilities only if both Ψ\Psi and the ψn\psi_n are normalised.
  • Writing ⟨p⟩=∫p ∣Ψ(x)∣2 dx\langle p\rangle = \int p\,|\Psi(x)|^2\,dx. There is no pp-value at each xx; use ⟨p⟩=∫Ψ∗(−iℏ∂x)Ψ dx\langle p\rangle = \int \Psi^*(-i\hbar\partial_x)\Psi\,dx, or work in momentum space with ∣Ψ~(p)∣2|\tilde\Psi(p)|^2.
  • Putting the operator in the wrong place. ⟨Q⟩=∫Ψ∗(Q^Ψ) dx\langle Q\rangle = \int \Psi^* (\hat Q\Psi)\,dx; Q^\hat Q acts on Ψ\Psi, then multiply by Ψ∗\Psi^*, then integrate.
  • Demanding ∂xΨ\partial_x\Psi be continuous at an infinite wall. Only Ψ\Psi is continuous there; its slope is allowed to jump because the potential is infinite.
  • Using a plane wave as a state. eikxe^{ikx} is not square-integrable; physical states are wave packets (normalisable superpositions of plane waves).
  • Confusing collapse with time evolution. The Schrödinger equation is deterministic and unitary; the random jump happens only at measurement.

Summary

  • State: a normalised complex Ψ(x,t)\Psi(x,t); Born rule: P(x) dx=∣Ψ∣2 dxP(x)\,dx = |\Psi|^2\,dx. Global phase is unphysical; amplitudes superpose.
  • Normalisation ∫∣Ψ∣2 dx=1\int|\Psi|^2\,dx = 1 is preserved by the dynamics, guaranteed by the continuity equation ∂tρ+∂xj=0\partial_t\rho + \partial_x j = 0 with j=ℏmIm(Ψ∗∂xΨ)j = \dfrac{\hbar}{m}\mathrm{Im}(\Psi^*\partial_x\Psi).
  • Observables are Hermitian operators: x^=x\hat x = x, p^=−iℏ ∂x\hat p = -i\hbar\,\partial_x; expectation value ⟨Q⟩=∫Ψ∗Q^Ψ dx\langle Q\rangle = \int \Psi^*\hat Q\Psi\,dx.
  • p^=−iℏ ∂x\hat p = -i\hbar\,\partial_x is forced by d⟨x⟩/dt=⟨p⟩/md\langle x\rangle/dt = \langle p\rangle/m; momentum eigenstates are eipx/ℏe^{ipx/\hbar} and ∣Ψ~(p)∣2|\tilde\Psi(p)|^2 is the momentum density.
  • Superposition Ψ=∑ncnψn\Psi = \sum_n c_n\psi_n; measurement returns qnq_n with probability ∣cn∣2|c_n|^2, cn=∫ψn∗Ψ dxc_n = \int\psi_n^*\Psi\,dx, then collapses the state to ψn\psi_n.
  • Admissible Ψ\Psi: single-valued, square-integrable, continuous, with continuous slope except at infinite potential features; Ψ→0\Psi\to0 at infinity.
  • The formalism is statistical: no trajectories, no explanation of individual outcomes, no local hidden variables.