math

commutator

An operator measuring the non-commutativity of two quantum operators, here of a scalar field.
25 related articles · 2 formulas

Description

In quantum mechanics, the commutator of two operators A and B is defined as [A, B] = AB - BA. It measures the degree to which the order of operations matters. If the commutator is zero, the operators commute, meaning their physical observables can be measured simultaneously with arbitrary precision. If it is non-zero, the operators do not commute, leading to fundamental uncertainty relations — the most famous being between position and momentum. In the context of a scalar field, the commutator of the field operator at two different spacetime points encodes the causal structure of the theory: if the points are spacelike separated, the commutator vanishes, ensuring that measurements at one point cannot influence the other, preserving relativity.

History

The concept of the commutator in quantum mechanics was introduced by Max Born and Pascual Jordan in 1925, and later formalized by Paul Dirac. The extension to quantum fields was developed in the late 1920s and 1930s by Werner Heisenberg, Wolfgang Pauli, and others.

How it works

For a scalar field φ(x), the commutator [φ(x), φ(y)] is not just a number but an operator. Its expectation value in the vacuum state gives a function that is zero when x and y are spacelike separated, and non-zero when they are timelike or lightlike separated. This property is derived from the field's equations of motion and the canonical commutation relations imposed at equal times. The commutator essentially tells you how a disturbance in the field at one point propagates to another: if the points are causally connected, the commutator is non-zero, reflecting the possibility of influence; if not, it is exactly zero, enforcing locality.

In practice

Commutators are fundamental to quantum field theory, where they are used to derive the Feynman propagator, which describes how particles move and interact. They also underpin the uncertainty principle, which is essential for understanding quantum measurement and the limits of precision in technologies like quantum cryptography.

Fun fact

The vanishing of the commutator for spacelike separations is so important that it is often called the 'microcausality' condition, and it is one of the few rigorous constraints that any relativistic quantum field theory must satisfy.

Concept graph →

Formulas

$$\frac{d\rho}{dt} = -\frac{i}{\hbar}[H,\rho] + \sum_n \left( L_n \rho L_n^\dagger - \frac{1}{2} \{ L_n^\dagger L_n, \rho \} \right)$$
Describes open quantum system evolution with dissipation.
What is in the formula
ρvariabledensity matrix of the open quantum system — density matrix
tvariabletime — time second
HvariableHamiltonian of the system — hamiltonian joule
L_nvariableLindblad operators (jump operators) for each dissipation channel — lindblad operator
iconstantimaginary unit, square root of -1 — imaginary unit = 1
ħconstantPlanck constant divided by 2π — reduced planck constant = 1.054571817e-34 joule second
d/dtoperatorderivative with respect to time — time derivative
[H, ρ]operatorcommutator of H and ρ — commutator
{L_n† L_n, ρ}operatoranticommutator of L_n† L_n and ρ — anticommutator
∑_noperatorsum over all dissipation channels — sum over channels
$$H_{ ext{eff}} = H_0 + rac{[H_{-1}, H_{+1}]}{ ext{frequency}}$$
Approximates the static Hamiltonian under high-frequency driving.
What is in the formula
H_effvariableeffective static Hamiltonian — hamiltonian joule
H_0variabletime-averaged Hamiltonian — hamiltonian joule
H_{-1}variablefirst negative Fourier component of the Hamiltonian — hamiltonian joule
H_{+1}variablefirst positive Fourier component of the Hamiltonian — hamiltonian joule
frequencyvariabledriving frequency — angular frequency radian per second
[ , ]operatormeasures the non-commutativity of two operators — commutator

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