Classicality parameter of a cosmological perturbation (source code)

= Classicality parameter of a cosmological perturbation

For a perturbation $X$, a normalized commutator
$$
\mathcal C=
\frac{|\langle[X,\dot X]\rangle|}
{\sqrt{\langle XX\rangle\langle\dot X\dot X\rangle}}
$$
compares its quantum commutator with its root-mean-square phase-space fluctuations. A limit $\mathcal C\to0$ signals effective classicality.