Quantum and Classical Liouville operators In the Heisenberg picture of Quantum Mechanics, for an observable $\hat{A}$, we have the famous Heisenberg equation giving the time evolution of the operator: ($\hat{H}$ is the Hamiltonian operator)
$$
i\hbar \frac{\partial \hat{A}}{\partial t} = -[\hat{H},\hat{A}]
$$
Which one can rewrite by defining the Lioville operator as:
$$
\hat{L}=\frac{1}{\hbar}[H,.]
$$
Thus
\begin{align}
\hat{A}(t) = e^{i\hat{L}t}\hat{A}(0) = e^{i\hat{H}t/\hbar}\hat{A}(0)e^{-i\hat{H}t/\hbar} \tag{1}
\end{align}
Similarly in classical statistical mechanics, for some classical differentiable variable $A$ we have the Poisson equation: ($H$ being the classical Hamiltonian here)
$$
\frac{\partial A}{\partial t} = \{A,H\}
$$
Now defining the classical version of the Liouville operator:
\begin{align}
\mathcal{L}:=i\{H,.\}=\sum_{i=1}^n [\frac{\partial H}{\partial p_i}\frac{\partial}{\partial q_i}-\frac{\partial H}{\partial q_i}\frac{\partial}{\partial p_i}] \tag{*}
\end{align}
Thus again defining the time evolution of $A$ with the corresponding propagator:
\begin{align}
A(t) = e^{i\mathcal{L}t}A(0) \tag{2}
\end{align}
Question:


*

*In $(1)$ we were able to further expand the unitary operator $e^{i\hat{L}t}$ into the two unitary time translations generated by $\hat{H}$ (sandwiching the value of the operator at time $t=0$), but looking at $(2)$, is there a way to further expand the propagator $e^{i\mathcal{L}t}$, using $(*)$, into a type of expression as was obtained in the QM version, namely equation $(1)$?

 A: OP's question (v1) is essentially asking

Does the operator identity
  $$ e^{\frac{it}{\hbar}[\hat{H},~\cdot~]}\hat{A}~ =~ e^{i\hat{H}t/\hbar}\hat{A}e^{-i\hat{H}t/\hbar} \tag{1} $$
  have an analog using functions/symbols $H$ and $A$ rather than operators $\hat{H}$ and $\hat{A}$, respectively? 

The answer is: Yes, in terms of the Groenewold-Moyal star product $\star$. If the Poisson bracket is written as
$$ \{A,B\}_{PB}~:=~A \stackrel{\leftarrow}{\partial_I} \omega^{IJ} \stackrel{\rightarrow}{\partial_J} B, \qquad \partial_I~\equiv~\frac{\partial}{\partial z^I}, \qquad  \{z^I,z^J\}_{PB}~=~\omega^{IJ},   \tag{2}  $$ 
where $z^1, \ldots, z^{2n}$ are canonical coordinates, and $A,B$ are functions/symbols (as opposed to operators), then the star product reads
$$ A\star B~:=~A \exp\left(\stackrel{\leftarrow}{\partial_I}\frac{i\hbar}{2} \omega^{IJ} \stackrel{\rightarrow}{\partial_J}\right) B~=~AB+\frac{i\hbar}{2}\{A,B\}_{PB} +{\cal O}(\hbar^2). \tag{3}  $$
And then an analog of eq. (1) is

$$ e^{\frac{it}{\hbar}[~H~\stackrel{\star}{,}~\cdot~]}A~=~ e_{\star}^{iHt/\hbar}\star A\star e_{\star}^{-iHt/\hbar}, \tag{4} $$

where 
$$[A\stackrel{\star}{,}B]~:= A\star B-B\star A~=~i\hbar\{A,B\}_{PB} +{\cal O}(\hbar^3)\tag{5} $$
is the star commutator, and
$$e_{\star}^B~:=~1+B\sum_{n=1}^{\infty}(\star B)^{n-1}/n!\tag{6} $$
is the star exponential. 
