I am reading about the sudden approximation in Sakurai. He writes the Schrodinger equation for the time evolution operator in terms of the variable t=sT: $$ i\frac{\partial}{\partial s}U(t,t_0)=\frac{H}{\hbar/T}U(t,t_0)=\frac{H}{\hbar\Omega}U(t,_t0)$$ with $\Omega=1/T$.
He then says that in the time scale $T\rightarrow 0$, $\hbar\Omega$ will be much larger than the energy scale represented by $H$. What is the energy scale represented by $H$? Is it its eigenvalues?
It also says that $T$ should be small compared to $2\pi/\omega_{ab}$ where $E{ab}=\hbar \omega_{ab}$ is the difference in energy between two relevant eigenvalues. But how do I know which are the relevant eigenvalues? And why is this condition required?