Will the Cosmos Expand Forever or Collapse?

  • Context: Graduate 
  • Thread starter Thread starter victorvmotti
  • Start date Start date
  • Tags Tags
    Cosmos
Click For Summary
SUMMARY

The discussion centers on the fate of the cosmos, specifically whether it will expand indefinitely or collapse. According to Carroll (2004), the cubic equation Ω0a^3+(1- ΩM0- Ω)a+ ΩM0=0 provides predictive power regarding the universe's expansion. Current observational data, when analyzed with standard Friedmann-Lemaître-Robertson-Walker models, strongly support a scenario of perpetual expansion rather than a "big crunch." The consensus is that the universe is near the borderline between open and closed, but the likelihood of collapse to a singular point in spacetime is dismissed due to the unidirectional nature of time.

PREREQUISITES
  • Understanding of cosmological models, specifically Friedmann-Lemaître-Robertson-Walker models
  • Familiarity with the concept of the scale factor in cosmology
  • Basic knowledge of cubic equations and their solutions
  • Awareness of the Hubble parameter and its significance in cosmology
NEXT STEPS
  • Research the implications of the Hubble parameter and its role in cosmic expansion
  • Study the derivation and applications of the Friedmann-Lemaître-Robertson-Walker equations
  • Explore the concept of dark energy and its impact on the universe's expansion
  • Investigate the historical context and evolution of the "big crunch" theory in cosmology
USEFUL FOR

Astronomers, cosmologists, and physics students interested in the long-term fate of the universe and the mathematical models that describe cosmic expansion.

victorvmotti
Messages
152
Reaction score
5
Will the cosmos expand forever or the expansion will stop and then the whole universe collapses to that point of spacetime from which the big bang started?

Carroll (2004) shows that this will become clear in a formula that shows the fate of the cosmos:

Ω0a^3+(1- ΩM0- Ω)a+ ΩM0=0

This simple cubic equation in terms of a, the scale factor, gives us predictive power. If there is no real solution to it then we have to expect “perpetual” expansion. And the current experimental data indeed favor such an open ended cosmic future.

What do you think about this conclusion?
 
Last edited:
Space news on Phys.org
I am not sure what it is that you are asking.

Yes, observational evidence, when combined standard Friedmann-Lemaitre-Robertson-Walker models, strongly favours a universe that expands forever.

The same observation evidence and models, however, make no strong prediction about whether the universe is open or closed, i.e.., the universe seems to be very near the borderline.
 
victorvmotti said:
Will the cosmos expand forever or the expansion will stop and then the whole universe collapses to that point of spacetime from which the big bang started?

It can't possibly collapse to the same point in spacetime where it started because the arrow of time only goes one way.

The "big crunch" scenario was in favor before accelerated expansion was discovered a couple of decades ago but is now widely regarded as not what's going to happen.

EDIT: I should add that the term "point in spacetime" should, I think, be taken to mean not just a particular point in time but also a particular point in space and since the big bang did not happen at a point in space, that's another reason why saying that it could go back to the "same" point in spacetime is impossible.
 
victorvmotti said:
This simple cubic equation in terms of a, the scale factor, gives us predictive power. If there is no real solution to it then we have to expect “perpetual” expansion. And the current experimental data indeed favor such an open ended cosmic future.
What do you think about this conclusion?
I think that every cubic equation has a real solution.
 
Bill_K said:
I think that every cubic equation has a real solution.

Carroll should have specified explicitly that turn-around values of the scale factor ##a## need to be real and positive, i.e., only positive solutions of the cubic are physically valid. He produces the real, positive solutions.
 
Last edited:
Great feedback.

Yes, he begins by seeing when the Hubble parameter passes through zero, changes sign, from positive to negative, and then arrives at this cubic equation in terms of the scale factor.

I was wondering if this cubic equation captures all information and related values, here only density parameters of matter and vacuum, to predict the fate of the cosmos, either a crunch or a perpetual expansion.
 

Similar threads

  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 4 ·
Replies
4
Views
4K
  • · Replies 13 ·
Replies
13
Views
6K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 27 ·
Replies
27
Views
4K
  • · Replies 3 ·
Replies
3
Views
3K
Replies
21
Views
4K
  • · Replies 7 ·
Replies
7
Views
3K
  • · Replies 12 ·
Replies
12
Views
5K
  • · Replies 62 ·
3
Replies
62
Views
11K