What Insights Does the Friedmann Equation Offer About Our Universe?

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SUMMARY

The Friedmann Equation provides critical insights into the dynamics of the universe, particularly regarding its curvature and potential recollapse. Discussions highlight that a closed universe, characterized by positive curvature (K_0), does not inherently indicate recollapse, especially when a nonzero cosmological constant (Λ) is considered. Traditional treatments often overlook this complexity, leading to misconceptions about the behavior of closed and open models. The conversation emphasizes the importance of advanced models that incorporate Λ to fully understand cosmological outcomes.

PREREQUISITES
  • Understanding of the Friedmann Equations
  • Familiarity with cosmological constants (Λ)
  • Knowledge of curvature in cosmology (positive, flat, and negative)
  • Basic principles of relativistic cosmology
NEXT STEPS
  • Research advanced cosmological models incorporating nonzero cosmological constants (Λ)
  • Study the implications of positive curvature (K_0) on universe dynamics
  • Learn about computational methods for solving the Friedmann Equations
  • Explore the relationship between curvature and universe recollapse scenarios
USEFUL FOR

Astronomers, physicists, and students of cosmology seeking to deepen their understanding of the Friedmann Equation and its implications for the universe's structure and fate.

Arman777
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Greg Bernhardt submitted a new PF Insights post

A Journey Into the Cosmos - The Friedmann Equation
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Continue reading the Original PF Insights Post.
 

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Great start @Arman777. This is part of our student series. If anyone has suggestions or feedback for him he would appreciate it!
 
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Very nice!
 
Drakkith said:
Very nice!
Thanks a lot :)
 
Very interesting post, one that even someone with an art major's understanding of physics can follow along. Like me, heh.

Inre to figure 8 and the crunch; years ago I came across a paper about solving the Friedmann equations by computer and noticed some surprising results. Surprising to me anyway. What do you think of their statement on page 2 --Thus a closed universe, by definition, is one with positive curvature K_0. Closure by itself does not tell us whether or not the universe will recollapse. In Sect. III we will show that in relativistic cosmology some open models recollapse and some closed ones do not."​
 
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chasrob said:
What do you think of their statement on page 2

It's true if there is a nonzero cosmological constant. Most introductory treatments of the Friedmann equations don't consider this case. If the cosmological constant is zero, then a closed universe will always recollapse and a flat or open one will always expand forever; that's why you often see statements along those lines in introductory treatments.
 
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chasrob said:
Very interesting post, one that even someone with an art major's understanding of physics can follow along. Like me, heh.[/I]"​

Thanks for your review, that was my purpose of writing this article.

chasrob said:
Inre to figure 8 and the crunch; years ago I came across a paper about solving the Friedmann equations by computer and noticed some surprising results. Surprising to me anyway. What do you think of their statement on page 2 --Thus a closed universe, by definition, is one with positive curvature K_0. Closure by itself does not tell us whether or not the universe will recollapse. In Sect. III we will show that in relativistic cosmology some open models recollapse and some closed ones do not."​

As PeterDonis said, my case is for ##Λ=0##. But in the next chapters, I' ll introduce the ##Λ## and solve some models when ##Λ≠0##.
 
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