Well I'm reading Mukhanov & Winitzki's Introduction to quantum effects in gravity, and I got to the exercise 2.8 that ask to derive Heisenberg's equation of motion
\begin{equation} \frac{d\hat{A}}{dt} = - \frac{i}{\hbar} [\hat{A},\hat{H}] + \frac{\partial \hat{A}}{\partial t} \end{equation}
And there is a couple of identities earlier, the classic ones in this part of quantum mechanics i.e. $[\hat{q},f] = i\hbar\ \partial f / \partial p$ and $[\hat{p},f] = -i\hbar\ \partial f / \partial q$, where $f = f(\hat{p}, \hat{q})$. And also Hamilton's equations.
So I tried to solve that exercise only with commutators and the identities that the book has given to you at that point, without the tipical aproach that mix Schrödinger's picture (like some people do it here or here), and I couldn't get to anywhere.
So I as wondering if there's a way to solve it without requiring Schrödinger's picture.