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Operators and Observables | Physics

In the position representation:

x^=x,p^=ix\hat{x} = x, \quad \hat{p} = -i\hbar\frac{\partial}{\partial x}

These satisfy the canonical commutation relation:

[x^,p^]=i[\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=aa\hat{A}|a\rangle = a|a\rangle with aa=1\langle a|a\rangle = 1. Then:

aA^a=aaa=a\langle a|\hat{A}|a\rangle = a\langle a|a\rangle = a

Taking the complex conjugate:

aA^a=aA^a=aA^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=aa = a^* So aa is real. \blacksquare

Proof that eigenstates are orthogonal. Let A^a=aa\hat{A}|a\rangle = a|a\rangle and A^b=bb\hat{A}|b\rangle = b|b\rangle With aba \neq b:

bA^a=aba\langle b|\hat{A}|a\rangle = a\langle b|a\rangle

bA^a=A^ba=bba=bba\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:

(ab)ba=0(a - b)\langle b|a\rangle = 0

Since aba \neq bWe must have ba=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}:

σAσB12[A^,B^]\sigma_A \sigma_B \geq \frac{1}{2}|\langle[\hat{A}, \hat{B}]\rangle|

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

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

σxσp12i=2\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}:

σA2σB214[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 αα0\langle\alpha|\alpha\rangle \geq 0:

ψ(ΔA^iλΔB^)(ΔA^+iλΔB^)ψ0\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^]+λ2σB20= \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^])24σA2σB20(\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):

σA2σB214[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/π)1/4exp(mωx2/(2))\psi_0(x) = (m\omega/\pi\hbar)^{1/4}\exp(-m\omega x^2/(2\hbar)):

x=0,x2=2mω    σx=2mω\langle x \rangle = 0, \quad \langle x^2 \rangle = \frac{\hbar}{2m\omega} \implies \sigma_x = \sqrt{\frac{\hbar}{2m\omega}}

p=0,p2=mω2    σp=mω2\langle p \rangle = 0, \quad \langle p^2 \rangle = \frac{m\omega\hbar}{2} \implies \sigma_p = \sqrt{\frac{m\omega\hbar}{2}}

σxσp=2\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=ψA^ψ=ψA^ψdx\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:

dx^dt=p^m,dp^dt=Vx\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:

dA^dt=i[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^]=2ip^[\hat{p}^2, \hat{x}] = -2i\hbar\hat{p}:

dx^dt=i ⁣[p^22m,x^]=i2i2mp^=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^]=iV(x^)[V(\hat{x}), \hat{p}] = i\hbar\,V'(\hat{x}):

dp^dt=i[V(x^),p^]=Vx\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 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=aϕ    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=2(0110)\hat{S}_x = \frac{\hbar}{2}\begin{pmatrix}0&1\\1&0\end{pmatrix}.

Solution

det ⁣(2(a11a))=0    a21=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 ±/2\pm\hbar/2.

For a=+1a = +1: (1111)(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(11)|-\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.

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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 dp/dt=V/xd\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^=id/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/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.