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Operators and Observables

Attempt these from memory before reading.

  • What makes an operator an observable? Give the two conditions.
  • Compute [x^,p^]=x^p^−p^x^[\hat{x}, \hat{p}] = \hat{x}\hat{p} - \hat{p}\hat{x} acting on a smooth test function.
  • State the generalised uncertainty principle.
  • Define the expectation value, and say what it is not.
  • What is the difference between Hermitian and self-adjoint, in one sentence?

Check your answers against the text. The last prompt is the one that catches people, and it is the reason the page exists.

Motivation: why an observable needs a domain

Section titled “Motivation: why an observable needs a domain”

In finite-dimensional linear algebra, a Hermitian matrix is all you need. It has real eigenvalues and an orthonormal eigenbasis, so “measure A^\hat{A}” means “read off an eigenvalue and its weight” and the probabilities in the Born rule have somewhere to live.

Physics is not finite-dimensional. The position operator x^=x\hat{x} = x and the momentum operator p^=−iℏ d/dx\hat{p} = -i\hbar\,\mathrm{d}/\mathrm{d}x are defined on functions, and the set of functions on which a differential operator is defined is not incidental — it is part of the operator. Changing the domain changes the operator, and can change whether it has real eigenvalues at all.

This is not a technicality. The momentum operator on the half-line is Hermitian on its natural domain and is not self-adjoint, and self-adjointness is what the spectral theorem needs. The spectral theorem is what guarantees a complete family of spectral projections, and those projections are what “probability of outcome aa” is defined in terms of. Lose self-adjointness and the Born rule has nothing to be a statement about.

So the two conditions are:

  • Hermitian (symmetric): ⟨ϕ,A^ψ⟩=⟨A^ϕ,ψ⟩\langle\phi, \hat{A}\psi\rangle = \langle \hat{A}\phi, \psi\rangle for all ψ,ϕ\psi, \phi in the domain.
  • Self-adjoint: Hermitian and the domain equals the domain of A^†\hat{A}^\dagger.

On a finite-dimensional space, domains are everything, so the two coincide. On a Hilbert space of functions, they need not, and the difference is exactly where the interesting physics lives.

In the position representation:

x^=x,p^=−iℏ∂∂x\hat{x} = x, \quad \hat{p} = -i\hbar\frac{\partial}{\partial x}

These satisfy the canonical commutation relation:

[x^,p^]=iℏ[\hat{x}, \hat{p}] = i\hbar

4.2 General Properties of Hermitian Operators

Section titled “4.2 General Properties of Hermitian Operators”

Hermitian operators have real eigenvalues and orthogonal eigenstates — essential for observables.

Theorem 4.1. If A^\hat{A} is Hermitian, then:

  • All eigenvalues are real.
  • Eigenstates corresponding to distinct eigenvalues are orthogonal.
  • The eigenstates form a complete basis (for the space of physical states).

Proof that eigenvalues are real. Let A^∣a⟩=a∣a⟩\hat{A}|a\rangle = a|a\rangle with ⟨a∣a⟩=1\langle a|a\rangle = 1. Then:

⟨a∣A^∣a⟩=a⟨a∣a⟩=a\langle a|\hat{A}|a\rangle = a\langle a|a\rangle = a

Taking the complex conjugate:

⟨a∣A^∣a⟩∗=⟨a∣A^†∣a⟩=⟨a∣A^∣a⟩=a∗\langle a|\hat{A}|a\rangle^* = \langle a|\hat{A}^\dagger|a\rangle = \langle a|\hat{A}|a\rangle = a^*

Where the second equality uses A^=A^†\hat{A} = \hat{A}^\dagger. Therefore a=a∗a = a^* So aa is real. ■\blacksquare

Proof that eigenstates are orthogonal. Let A^∣a⟩=a∣a⟩\hat{A}|a\rangle = a|a\rangle and A^∣b⟩=b∣b⟩\hat{A}|b\rangle = b|b\rangle With a≠ba \neq b:

⟨b∣A^∣a⟩=a⟨b∣a⟩\langle b|\hat{A}|a\rangle = a\langle b|a\rangle ⟨b∣A^∣a⟩=⟨A^b∣a⟩=b∗⟨b∣a⟩=b⟨b∣a⟩\langle b|\hat{A}|a\rangle = \langle\hat{A}b|a\rangle = b^*\langle b|a\rangle = b\langle b|a\rangle

Where the last step uses b∗=bb^* = b (eigenvalues are real). Therefore:

(a−b)⟨b∣a⟩=0(a - b)\langle b|a\rangle = 0

Since a≠ba \neq b We must have ⟨b∣a⟩=0\langle b|a\rangle = 0. ■\blacksquare

Theorem 4.2 (Spectral Theorem). Every Hermitian operator on a finite-dimensional Hilbert space Has a complete orthonormal set of eigenvectors. In infinite dimensions, this holds for Self-adjoint operators with a discrete spectrum; operators with continuous spectra require the Spectral theorem in its general form (resolution of the identity).

The commutator of two operators is [A^,B^]=A^B^−B^A^[\hat{A}, \hat{B}] = \hat{A}\hat{B} - \hat{B}\hat{A}.

Theorem 4.3 (Generalised Uncertainty Principle). For observables A^\hat{A} and B^\hat{B}:

σAσB≥12∣⟨[A^,B^]⟩∣\sigma_A \sigma_B \geq \frac{1}{2}|\langle[\hat{A}, \hat{B}]\rangle|

Corollary 4.4 (Heisenberg Uncertainty Principle). σxσp≥ℏ/2\sigma_x \sigma_p \geq \hbar/2.

Proof. This follows from the generalised uncertainty principle with [x^,p^]=iℏ[\hat{x}, \hat{p}] = i\hbar:

σxσp≥12∣⟨iℏ⟩∣=ℏ2\sigma_x \sigma_p \geq \frac{1}{2}|\langle i\hbar \rangle| = \frac{\hbar}{2}

■\blacksquare

4.4 Proof of the Generalised Uncertainty Principle

Section titled “4.4 Proof of the Generalised Uncertainty Principle”

Theorem 4.5 (Robertson-Schrodinger inequality). For any state ∣ψ⟩|\psi\rangle and observables A^\hat{A}, B^\hat{B}:

σA2 σB2≥14∣⟨[A^,B^]⟩∣2+14⟨{ΔA^,ΔB^}⟩2\sigma_A^2\,\sigma_B^2 \geq \frac{1}{4}|\langle[\hat{A}, \hat{B}]\rangle|^2 + \frac{1}{4}\langle\{\Delta\hat{A}, \Delta\hat{B}\}\rangle^2

Where ΔA^=A^−⟨A^⟩\Delta\hat{A} = \hat{A} - \langle\hat{A}\rangle and σA2=⟨ΔA^2⟩\sigma_A^2 = \langle\Delta\hat{A}^2\rangle.

Proof. Define ∣α⟩=(ΔA^+iλΔB^)∣ψ⟩|\alpha\rangle = (\Delta\hat{A} + i\lambda\Delta\hat{B})|\psi\rangle for a real Parameter λ\lambda. Since ⟨α∣α⟩≥0\langle\alpha|\alpha\rangle \geq 0:

⟨ψ∣(ΔA^−iλΔB^)(ΔA^+iλΔB^)∣ψ⟩≥0\langle\psi|(\Delta\hat{A} - i\lambda\Delta\hat{B})(\Delta\hat{A} + i\lambda\Delta\hat{B})|\psi\rangle \geq 0 =σA2+iλ⟨[ΔA^,ΔB^]⟩+λ2σB2≥0= \sigma_A^2 + i\lambda\langle[\Delta\hat{A}, \Delta\hat{B}]\rangle + \lambda^2\sigma_B^2 \geq 0

This is a quadratic in λ\lambda that is non-negative for all λ\lambda So its discriminant must be non-positive:

(⟨[ΔA^,ΔB^]⟩)2−4σA2σB2≤0(\langle[\Delta\hat{A}, \Delta\hat{B}]\rangle)^2 - 4\sigma_A^2\sigma_B^2 \leq 0

Since [ΔA^,ΔB^]=[A^,B^][\Delta\hat{A}, \Delta\hat{B}] = [\hat{A}, \hat{B}] (constants commute with everything):

σA2 σB2≥14∣⟨[A^,B^]⟩∣2■\sigma_A^2\,\sigma_B^2 \geq \frac{1}{4}|\langle[\hat{A}, \hat{B}]\rangle|^2 \qquad \blacksquare

The stronger Robertson-Schrodinger form retains the anticommutator term ⟨{ΔA^,ΔB^}⟩2\langle\{\Delta\hat{A}, \Delta\hat{B}\}\rangle^2 Which is always non-negative and provides a tighter bound.

Example 4.1. Show that the uncertainty principle is saturated for the harmonic oscillator ground state.

Solution

For the ground state ψ0(x)=(mω/πℏ)1/4exp⁡(−mωx2/(2ℏ))\psi_0(x) = (m\omega/\pi\hbar)^{1/4}\exp(-m\omega x^2/(2\hbar)):

⟨x⟩=0,⟨x2⟩=ℏ2mω  ⟹  σx=ℏ2mω\langle x \rangle = 0, \quad \langle x^2 \rangle = \frac{\hbar}{2m\omega} \implies \sigma_x = \sqrt{\frac{\hbar}{2m\omega}} ⟨p⟩=0,⟨p2⟩=mωℏ2  ⟹  σp=mωℏ2\langle p \rangle = 0, \quad \langle p^2 \rangle = \frac{m\omega\hbar}{2} \implies \sigma_p = \sqrt{\frac{m\omega\hbar}{2}} σx σp=ℏ2\sigma_x\,\sigma_p = \frac{\hbar}{2}

This saturates the Heisenberg bound, so the ground state is a minimum uncertainty state (Gaussian).

The expectation value of an observable A^\hat{A} in state ∣ψ⟩|\psi\rangle:

⟨A⟩=⟨ψ∣A^∣ψ⟩=∫ψ∗A^ψ dx\langle A \rangle = \langle \psi | \hat{A} | \psi \rangle = \int \psi^* \hat{A} \psi\, dx

Theorem 4.6 (Ehrenfest’s Theorem). Quantum expectation values obey classical equations of motion:

d⟨x^⟩dt=⟨p^⟩m,d⟨p^⟩dt=−⟨∂V∂x⟩\frac{d\langle \hat{x} \rangle}{dt} = \frac{\langle \hat{p} \rangle}{m}, \quad \frac{d\langle \hat{p} \rangle}{dt} = -\left\langle \frac{\partial V}{\partial x}\right\rangle

Proof of Ehrenfest’s Theorem. From the Schrodinger equation:

d⟨A^⟩dt=iℏ⟨[H^,A^]⟩+⟨∂A^∂t⟩\frac{d\langle \hat{A} \rangle}{dt} = \frac{i}{\hbar}\langle[\hat{H}, \hat{A}]\rangle + \left\langle\frac{\partial \hat{A}}{\partial t}\right\rangle

For A^=x^\hat{A} = \hat{x} (no explicit time dependence), using [p^2,x^]=−2iℏp^[\hat{p}^2, \hat{x}] = -2i\hbar\hat{p}:

d⟨x^⟩dt=iℏ ⁣⟨[p^22m,x^]⟩=iℏ⋅−2iℏ2m⟨p^⟩=⟨p^⟩m\frac{d\langle \hat{x} \rangle}{dt} = \frac{i}{\hbar}\!\left\langle\left[\frac{\hat{p}^2}{2m}, \hat{x}\right]\right\rangle = \frac{i}{\hbar}\cdot\frac{-2i\hbar}{2m}\langle\hat{p}\rangle = \frac{\langle\hat{p}\rangle}{m}

For A^=p^\hat{A} = \hat{p} Using [V(x^),p^]=iℏ V′(x^)[V(\hat{x}), \hat{p}] = i\hbar\,V'(\hat{x}):

d⟨p^⟩dt=iℏ⟨[V(x^),p^]⟩=−⟨∂V∂x⟩\frac{d\langle \hat{p} \rangle}{dt} = \frac{i}{\hbar}\langle[V(\hat{x}), \hat{p}]\rangle = -\left\langle\frac{\partial V}{\partial x}\right\rangle

■\blacksquare

Correspondence principle. Ehrenfest’s theorem embodies the correspondence principle: in the Classical limit (large quantum numbers or ℏ→0\hbar \to 0), quantum expectation values follow Classical trajectories. However, this is only exact for linear or quadratic potentials; for general Potentials, ⟨V′(x)⟩≠V′(⟨x⟩)\langle V'(x) \rangle \neq V'(\langle x \rangle) So quantum corrections persist even for large systems.

To find the eigenvalues and eigenvectors of an operator A^\hat{A} Solve:

A^∣ϕ⟩=a∣ϕ⟩  ⟹  det⁡(A^−aI^)=0\hat{A}|\phi\rangle = a|\phi\rangle \implies \det(\hat{A} - a\hat{I}) = 0

The roots give the eigenvalues; substituting each back yields the eigenvectors.

Example 4.3. Find the eigenvalues and eigenvectors of S^x=ℏ2(0110)\hat{S}_x = \frac{\hbar}{2}\begin{pmatrix}0&1\\1&0\end{pmatrix}.

Solutiondet⁡ ⁣(ℏ2(−a11−a))=0  ⟹  a2−1=0  ⟹  a=±1\det\!\left(\frac{\hbar}{2}\begin{pmatrix}-a & 1\\1 & -a\end{pmatrix}\right) = 0 \implies a^2 - 1 = 0 \implies a = \pm 1

Eigenvalues are ±ℏ/2\pm\hbar/2.

For a=+1a = +1: (−111−1)(c1c2)=0  ⟹  c1=c2\begin{pmatrix}-1 & 1\\1 & -1\end{pmatrix}\begin{pmatrix}c_1\\c_2\end{pmatrix} = 0 \implies c_1 = c_2. Normalised: ∣+⟩x=12(11)|+\rangle_x = \frac{1}{\sqrt{2}}\begin{pmatrix}1\\1\end{pmatrix}.

For a=−1a = -1: c1=−c2c_1 = -c_2. Normalised: ∣−⟩x=12(1−1)|-\rangle_x = \frac{1}{\sqrt{2}}\begin{pmatrix}1\\-1\end{pmatrix}.

These are equal superpositions of the SzS_z eigenstates. Note that measuring SxS_x on a state of Definite SzS_z gives probabilistic outcomes, and vice versa.

Quantum operators are the bridge between abstract mathematical states and physical measurements. Each observable, such as position or momentum, is represented by an operator whose eigenvalues are the possible outcomes you could measure. Operators for incompatible observables do not commute, which means measuring one precisely forces the other to become uncertain. This is not a limitation of instruments but a fundamental feature of quantum reality. Ehrenfest’s theorem shows that quantum expectation values follow classical equations of motion on average, providing a smooth bridge from quantum to classical behaviour. Spin-half systems illustrate these ideas most vividly.

Mistake 1: Assuming ⟨V′(x)⟩=V′(⟨x⟩)\langle V'(x) \rangle = V'(\langle x \rangle) in Ehrenfest’s theorem Ehrenfest’s theorem gives d⟨p⟩/dt=−⟨∂V/∂x⟩d\langle p \rangle/dt = -\langle \partial V/\partial x \rangle, not −V′(⟨x⟩)-V'(\langle x \rangle). The expectation value of the derivative of VV is generally not the derivative of VV at the expectation value. This equality holds only for linear or quadratic potentials. Students frequently make this substitution when applying Ehrenfest’s theorem to anharmonic oscillators.

Mistake 2: Confusing Hermitian operators with self-adjoint operators Every self-adjoint operator is Hermitian, but the converse is not true for operators on infinite-dimensional spaces. The momentum operator p^=−iℏ d/dx\hat{p} = -i\hbar\,d/dx is Hermitian on a dense domain but may fail to be self-adjoint depending on boundary conditions. Self-adjointness requires the domain of A^\hat{A} and A^†\hat{A}^\dagger to coincide, which is essential for the spectral theorem.

Mistake 3: Assuming the uncertainty principle limits measurement precision The Heisenberg uncertainty principle σxσp≥ℏ/2\sigma_x \sigma_p \geq \hbar/2 is a property of quantum states, not a limitation of measurement apparatus. It reflects the inherent spread of a state in position and momentum space simultaneously. A minimum-uncertainty Gaussian state saturates the bound, showing it is a fundamental feature of quantum mechanics, not an instrumental error.

Quantum operators are the machinery that extracts measurable information from a quantum state. Each observable, like position or momentum, has an associated operator whose eigenvalues are the possible measurement outcomes. The expectation value of an operator gives the average result over many identical measurements. Commuting operators share eigenstates, meaning both observables can be known simultaneously. Non-commuting operators, like position and momentum, obey an uncertainty relation: measuring one precisely forces the other to become uncertain. This is not a limitation of instruments but a fundamental feature of quantum reality. Spin-half systems illustrate this vividly: measuring spin along one axis gives random results for the orthogonal axis.

ClaimTrue?Counterexample
Hermitian is the same as self-adjointnop^=−iℏ d/dx\hat{p} = -i\hbar\,\mathrm{d}/\mathrm{d}x on the half-line is Hermitian on its natural domain and admits no self-adjoint extension without a boundary condition added
Every observable has a complete set of eigenstatesnonot for a general Hermitian operator; it is true for self-adjoint ones, and position and momentum have a continuous spectrum rather than a countable one
Commuting observables can be measured simultaneously with arbitrary precisionnocommuting self-adjoint operators may have no common eigenbasis; what follows from [A^,B^]=0[\hat{A},\hat{B}] = 0 is a common invariant subspace
Eigenvalues of an observable are distinctnodegeneracy is ubiquitous and physical — spin multiplets and atomic levels — and is not a defect
The expectation value is the value you will measurenoit is the mean over many identically prepared systems; a single measurement returns an eigenvalue
The uncertainty principle limits how well instruments can measurenoit bounds the spread of a state, and is attained by minimum-uncertainty Gaussians, so it is not an instrumental error
Every observable has a discrete spectrumnox^\hat{x} and p^\hat{p} have continuous spectra; the generalised eigenfunctions are distributions, not vectors
An operator is defined by its formulanoit is defined by its formula and its domain; the same formula on different domains is a different operator

The first row is the one that matters most, and it is also the one that feels like pedantry until you meet an example. The last row is its general form and is worth internalising: on an infinite-dimensional space, writing the operator down is only half the specification.

The third row deserves emphasis. The common statement is “commuting observables are simultaneously measurable”, and it is a theorem about a common eigenspace — which need not be the whole space. Two operators can commute and still leave you unable to assign both eigenvalues at once.

  • Domains in quantum mechanics. Whether the Hamiltonian admits a self-adjoint extension is a genuine mathematical question with physical answers: boundary conditions at a singular endpoint can make the extension unique, absent, or a family parameterised by an angle, and that angle is the quantum number.
  • Observables without spectra. Quantum field theory has no eigenvalues to read. The observable algebra is local and relativistic, and the theory of von Neumann algebras replaces “operator with spectrum” with “local algebra with representations”.
  • Haag’s theorem. Local relativistic observables cannot be unitarily equivalent to the free field ones. It is a rigorous statement that the mathematical frame of canonical quantisation breaks down in QFT, and reconciling it remains open.
  • Generalised measurement theory. POVMs generalise projective measurements; whether they describe real apparatus or are a mathematical convenience is still argued.
  • Black-hole information and observables. Which operators count as observables inside a black hole, and what algebra they satisfy, is unsettled and empirically constrained.

Mix these with the postulates, wave functions, spin, Linear Algebra, Functional Analysis and Spectral Theory.

  1. (Linear algebra.) Prove that a Hermitian operator on a finite-dimensional space has an orthonormal eigenbasis. Identify every step of the proof that fails in infinite dimensions, and say which hypothesis each one used.
  2. (Functional analysis.) State the spectral theorem for self-adjoint operators, and explain why the theorem is false for merely Hermitian ones. Then take the first derivative on L2(0,1)L^2(0,1) and determine its adjoint, checking domains rather than formal expressions.
  3. (Wave functions.) Compute [x^,p^][\hat{x}, \hat{p}] acting on a smooth compactly supported function by differentiating, with no appeal to a formula. Then say why the answer is iℏi\hbar rather than the classical commutator 00, and what that statement means physically.
  4. (Spectral theory.) Show that the spectral measure of p^\hat{p} is Lebesgue measure, using the Fourier transform: the projectors of p^\hat{p} are the Fourier projections onto sets. What does it mean that position and momentum have continuous spectral measures rather than countable ones?
  5. (Linear algebra.) Two Hermitian operators commute. Show that every eigenvector of one is an eigenvector of the other if the eigenvalues of the first are non-degenerate, and construct a two-dimensional example with degenerate eigenvalues where the conclusion fails.
  6. (Research.) State Haag’s theorem in the form that local, covariant, time-ordered algebras cannot be unitarily equivalent to the free-field algebra. Explain what it implies about canonical quantisation, and why it is not regarded as showing QFT is inconsistent.