WMAP and Big Crunch: Is the Universe's Fate Sealed?

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SUMMARY

The WMAP survey results confirm that the average energy density of the universe is equal to the critical density, represented as Ω = 1. This measurement indicates that the universe is on the threshold between eternal expansion and eventual contraction. The presence of dark energy complicates this scenario, as it exerts a pressure that can lead to perpetual expansion even if the energy density is slightly above critical. Therefore, the possibility of a "big crunch" is effectively ruled out under current understanding.

PREREQUISITES
  • Understanding of cosmological principles, specifically critical density.
  • Familiarity with dark energy and its effects on cosmic expansion.
  • Knowledge of the WMAP survey and its significance in cosmology.
  • Basic grasp of energy density equations in cosmology.
NEXT STEPS
  • Research the implications of dark energy on cosmic expansion.
  • Study the WMAP survey findings in detail, focusing on energy density measurements.
  • Explore mathematical models predicting universe behavior under varying energy densities.
  • Investigate alternative theories to the big crunch scenario in cosmology.
USEFUL FOR

Astronomers, cosmologists, and physics students interested in the fate of the universe and the implications of dark energy on cosmic evolution.

vincentm
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Hello all,

With the results of the WMAP survery of the CMB back in march of this year, has this ruled out the possibility of the universe undergoing a "big crunch"?

I've read somewhere that the average density of matter in the universe has been measured to be

p=1

Is this right?
 
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In an universe without dark energy, an average energy density above the critical density would lead to a big-crunch, and an average energy density below or equal to the critial density would lead to an eternal expansion. However, with dark energy things are different. An universe with average energy density above the critical density may expand forever. This is because dark energy exterts a pressure that accelerates the expansion of space.

The average energy density measured by WMAP is equal to the critical density [itex]\Omega = \rho / \rho_{crit} = 1[/itex]. Even if it would be slightly above the critical energy density, our universe would expand forever. I remember that a time ago I tried some calculations to find out what is the lowest value for the relation between the energy density of matter and the energy density of dark energy (assuming it to be a cosmological constant) for which a closed expanding universe will start contracting: if there is enough matter the expanding universe will start contracting regardless of the effect of dark energy and before it starts becoming dominant. I could not find this calculations now, but if you are interested we could try to figure it out.
 
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