Big crunch versus the Cosmological Constant

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The discussion centers on the contrasting theories of the universe's fate: the big crunch versus the cosmological constant. While the big crunch suggests a future contraction of the universe, current observations indicate that the universe is expanding at an accelerating rate due to the cosmological constant. This acceleration points towards a potential heat death scenario rather than a big crunch, as it leads to thermal equilibrium in open and flat universes. The nature of dark energy, which drives this accelerated expansion, remains uncertain, particularly whether it is a constant or has time-dependent properties. If dark energy were to change, the ultimate fate of the universe could shift, potentially leading to a big crunch if the universe is closed.
zheng89120
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I am no expert on cosmology. But from what I have heard, the big crunch is the scenario that will most likely happen to our universe in the (far) future. Yet the cosmological constant makes it so that our universe is currently expanding and acceleratingly so. So the question is (I know this may not be that hard to imagine), how is the fact that our universe will de-accelerate and contract in time to be reconciled with the fact that it is expanding from the cosmological constant. Thanks.
 
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It appears the big crunch is less likely than the big chill, based on current cosmological data. It appears expansion was slowing until about the time Earth formed. Since then, it appears to be accelerating.
 
zheng89120 said:
So the question is (I know this may not be that hard to imagine), how is the fact that our universe will de-accelerate and contract in time to be reconciled with the fact that it is expanding from the cosmological constant. Thanks.
You are exactly right! As Chronos says, the accelerated expansion appears to be leading the universe to a rather different fate than a big crunch. Heat death, in which the universe eventually reaches thermal equilibrium, is the ultimate fate of all open and flat universes. Throw in a cosmological constant and it becomes possible to attain heat death even in closed models. Of course, the universe could throw us another curve ball at some point in the future. We currently don't understand the nature of the dark energy that's driving the accelerated expansion, in particular, we don't know whether it's a true constant or whether it has a time dependance. If it is time dependent, it might decay at some point and then the fate of the universe will be left in the hands of its curvature: if it's closed, we get a big crunch; otherwise, heat death.
 
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