--- title: "Rotating wave approximation" date: 2022-02-01 categories: - Physics - Quantum mechanics - Two-level system - Optics layout: "concept" --- Consider the following periodic perturbation $\hat{H}_1$ to a quantum system, which represents e.g. an [electromagnetic wave](/know/concept/electromagnetic-wave-equation/) in the [electric dipole approximation](/know/concept/electric-dipole-approximation/): $$\begin{aligned} \hat{H}_1(t) = \hat{V} \cos(\omega t) = \frac{\hat{V}}{2} \Big( e^{i \omega t} + e^{-i \omega t} \Big) \end{aligned}$$ Where $\hat{V}$ is some operator, and we assume that $\omega$ is fairly close to a resonance frequency $\omega_0$ of the system that is getting perturbed by $\hat{H}_1$. As an example, consider a two-level system consisting of states $\Ket{g}$ and $\Ket{e}$, with a resonance frequency $\omega_0 = (E_e \!-\! E_g) / \hbar$. From the derivation of [time-dependent perturbation theory](/know/concept/time-dependent-perturbation-theory/), we know that the state $\Ket{\Psi} = c_g \Ket{g} + c_e \Ket{e}$ evolves as: $$\begin{aligned} i \hbar \dv{c_g}{t} &= \matrixel{g}{\hat{H}_1(t)}{g} \: c_g(t) + \matrixel{g}{\hat{H}_1(t)}{e} \: c_e(t) \: e^{- i \omega_0 t} \\ i \hbar \dv{c_e}{t} &= \matrixel{e}{\hat{H}_1(t)}{g} \: c_g(t) \: e^{i \omega_0 t} + \matrixel{e}{\hat{H}_1(t)}{e} \: c_e(t) \end{aligned}$$ Typically, $\hat{V}$ has odd spatial parity, in which case [Laporte's selection rule](/know/concept/selection-rules/) reduces this to: $$\begin{aligned} \dv{c_g}{t} &= \frac{1}{i \hbar} \matrixel{g}{\hat{H}_1}{e} \: c_e \: e^{- i \omega_0 t} \\ \dv{c_e}{t} &= \frac{1}{i \hbar} \matrixel{e}{\hat{H}_1}{g} \: c_g \: e^{i \omega_0 t} \end{aligned}$$ We now insert the general $\hat{H}_1$ defined above, and define $V_{eg} \equiv \matrixel{e}{\hat{V}}{g}$ to get: $$\begin{aligned} \dv{c_g}{t} &= \frac{V_{eg}^*}{i 2 \hbar} \Big( e^{i (\omega - \omega_0) t} + e^{- i (\omega + \omega_0) t} \Big) \: c_e \\ \dv{c_e}{t} &= \frac{V_{eg}}{i 2 \hbar} \Big( e^{i (\omega + \omega_0) t} + e^{- i (\omega - \omega_0) t} \Big) \: c_g \end{aligned}$$ At last, here we make the **rotating wave approximation**: since $\omega$ is assumed to be close to $\omega_0$, we argue that $\omega \!+\! \omega_0$ is so much larger than $\omega \!-\! \omega_0$ that those oscillations turn out negligible if the system is observed over a reasonable time interval. Specifically, since both exponentials have the same weight, the fast ($\omega \!+\! \omega_0$) oscillations have a tiny amplitude compared to the slow ($\omega \!-\! \omega_0$) ones. Furthermore, since they average out to zero over most realistic time intervals, the fast terms can be dropped, leaving: $$\begin{aligned} \boxed{ \begin{aligned} e^{i (\omega - \omega_0) t} + e^{- i (\omega + \omega_0) t} &\approx e^{i (\omega - \omega_0) t} \\ e^{i (\omega + \omega_0) t} + e^{- i (\omega - \omega_0) t} &\approx e^{- i (\omega - \omega_0) t} \end{aligned} } \end{aligned}$$ Such that our example set of equations can be approximated as shown below, and its analysis can continue; see [Rabi oscillation](/know/concept/rabi-oscillation/) for more: $$\begin{aligned} \dv{c_g}{t} &= \frac{V_{eg}^*}{i 2 \hbar} c_e \: e^{i (\omega - \omega_0) t} \\ \dv{c_e}{t} &= \frac{V_{eg}}{i 2 \hbar} c_g \: e^{- i (\omega - \omega_0) t} \end{aligned}$$ This approximation's name is a bit confusing: the idea is that going from the Schrödinger to the [interaction picture](/know/concept/interaction-picture/) has the effect of removing the exponentials of $\omega_0$ from the above equations, i.e. multiplying them by $e^{i \omega_0 t}$ and $e^{- i \omega_0 t}$ respectively, which can be regarded as a rotation. Relative to this rotation, when we split the wave $\cos(\omega t)$ into two exponentials, one co-rotates, and the other counter-rotates. We keep only the co-rotating waves, hence the name. The rotating wave approximation is usually used in the context of the two-level quantum system for light-matter interactions, as in the above example. However, it is not specific to that case, and it more generally refers to any approximation where fast-oscillating terms are neglected.