That’s different from inflation, though possibly related. Yes, if the expansion were Newtonian, then the rate should be slowing down (it may or may not be slowing down enough to eventually stop, but it should be slowing down at least some), but as you say, that’s not what we observe. So, why is the expansion accelerating? The answer is dark energy, but that’s really no answer at all. “Dark energy” is just a label we put on the unknown cause of the acceleration.
What is it actually, and how does it work? On that point, we’re worse than clueless. I say “worse than clueless”, because we do actually have a clue, it’s just a horrendously bad one: Particle physics models predict that there should be something called the vacuum energy, which should behave qualitatively in the right way to be the dark energy. Qualitatively, but not quantitatively: Our particle physics models aren’t yet good enough to calculate the exact strength of the vacuum energy, but we can at least estimate it… And those estimates turn out to be 120 orders of magnitude larger than what we observe. Note: That’s not a factor of 120, that’s a factor of 10^120. So, is the dark energy vacuum energy? Maybe, but if so, it’s got a lot of 'splainin to do.
What of inflation, then? Well, our best cosmological models say that in the very early stages of the Universe, it should have been expanding (and accelerating) at a much greater rate than it is today. In fact, the early rate of acceleration really does seem like it’d be consistent with the predictions for vacuum energy. And then, for reasons that we don’t entirely understand, that super-fast early expansion stopped.
So, are the dark energy and inflation two different manifestations of the same sort of phenomenon? If so, why did its strength change so radically? Are they two completely unrelated phenomena? Then what’s the dark energy, and why did inflation end? Are they separate phenomena, but somehow related? How? We really do have a lot more questions than answers, here.