An operator measuring the non-commutativity of two quantum operators, here of a scalar field.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.
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.
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.
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.
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.
| ρ | variable | density matrix of the open quantum system — density matrix |
| t | variable | time — time second |
| H | variable | Hamiltonian of the system — hamiltonian joule |
| L_n | variable | Lindblad operators (jump operators) for each dissipation channel — lindblad operator |
| i | constant | imaginary unit, square root of -1 — imaginary unit = 1 |
| ħ | constant | Planck constant divided by 2π — reduced planck constant = 1.054571817e-34 joule second |
| d/dt | operator | derivative with respect to time — time derivative |
| [H, ρ] | operator | commutator of H and ρ — commutator |
| {L_n† L_n, ρ} | operator | anticommutator of L_n† L_n and ρ — anticommutator |
| ∑_n | operator | sum over all dissipation channels — sum over channels |
| H_eff | variable | effective static Hamiltonian — hamiltonian joule |
| H_0 | variable | time-averaged Hamiltonian — hamiltonian joule |
| H_{-1} | variable | first negative Fourier component of the Hamiltonian — hamiltonian joule |
| H_{+1} | variable | first positive Fourier component of the Hamiltonian — hamiltonian joule |
| frequency | variable | driving frequency — angular frequency radian per second |
| [ , ] | operator | measures the non-commutativity of two operators — commutator |












