marcus
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Stephanus said:And...?
What if the Hubble constant go down even <0?
The big crunch?
That is right, as a "what if". In models where the universe contracts the H is negative. But the change in H has been observed over time and the evidence is that although it has indeed been decreasing it is not tending to zero, or into negative territory! It is leveling out at a positive value.
(that is what is beginning to cause acceleration in individual distance growth speeds)
You can see the leveling out in the plot.