Chalnoth
Science Advisor
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I think you're a bit confused between the rate of expansion H and the acceleration of the scale factor, a(t).Myslius said:Correct. Just when you see the increase in the rate of expansion that increase was billions of years ago, not now. If you want to know how the rate of expansion changed (or will change) over time you have to reverse the timescale.
The rate of expansion H has always been decreasing. However, lately it has been decreasing more slowly, slowly enough that it leads to an accelerating expansion. How is this possible? Well, the rate of expansion H is defined as:
H(t) = {1 \over a(t)}{da(t) \over dt}
I think the easiest way to see why a slowly-decreasing H(t) leads to an accelerating expansion is to consider a constant H(t) = H_0.
H_0 = {1 \over a(t)}{da(t) \over dt}
{da(t) \over dt} = H_0 a(t)
So a constant rate of expansion H(t) means that change in the scale factor is proportional to the scale factor: this is exponential growth! Specifically:
a(t) = a(t=0) e^{H_0 t}
So a constant rate of expansion means that objects within the universe are accelerating away from one another exponentially fast. This isn't the situation we're in yet, but it appears that our universe is approaching this situation.