The identity $\hat{U} = e^{- \frac{i}{\hbar} \hat{H} t}$ holds only for a time-independent hamiltonian, which does not apply here. Instead, the propagator here is given by the time-ordered exponential $\hat{U}(t_2,t_1) = \mathcal T \left[e^{- \frac{i}{\hbar} \int_{t_1}^{t_2} \hat{H}(t) \mathrm d t}\right]$, which is not particularly useful in this situation.
In your situation, you've got very few options left to you other than direct solution of the coupled Schrödinger equations,
\begin{align}
i\hbar \dot a(t) & = E_0e^{t/w_0} a(t) + E_1 b(t), \\
i\hbar \dot b(t) & = E_1 a(t) + E_0e^{t/w_0} b(t).
\end{align}
This one is hard to solve but you can make a start by setting $E_1=0$, in which case both $a$ and $b$ obey the differential equation
$$
i\hbar \dot c(t) = E_0e^{t/w_0} c(t),
$$
whose solution is
$$
c(t)= c(0)e^{-i e^{t/w_0}E_0 w_0/\hbar},
$$
so you can ride on that and define $a(t) = \alpha(t) e^{-i e^{t/w_0}E_0 w_0/\hbar}$ and $b(t) = \beta(t) e^{-i e^{t/w_0}E_0 w_0/\hbar}$, for which the Schrödinger equation simplifies to
\begin{align}
i\hbar \dot \alpha(t) & =E_1 \beta(t) , \\
i\hbar \dot \beta(t) & = E_1 \alpha(t) ,
\end{align}
whose solutions are
\begin{align}
\alpha(t) & = \alpha(0) \cos(E_1t/\hbar) -i \beta(0) \sin(E_1t/\hbar)\\
\beta(t) & = -i\alpha(0) \sin(E_1t/\hbar) + \beta(0) \cos(E_1t/\hbar).
\end{align}
Anything beyond that will depend on exactly what you want to do with those solutions.