Why Does Cosmic Growth End and Why Is Our Era Unique?

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SUMMARY

The discussion centers on the paper "The End of Cosmic Growth" by Eric V. Linder and David Polarski, which explores the dynamics of cosmic structure growth under general relativity (GR) and modified gravity. It concludes that gravitational attraction is ultimately overcome by cosmic acceleration, leading to the cessation of growth in large-scale structures. The authors highlight a unique temporal aspect of our era, where the gravitational growth index γ indicates a significant transition point between past and future behaviors. The conversation also critiques the title of the thread, emphasizing that the focus is on the end of structural growth rather than cosmic expansion.

PREREQUISITES
  • Understanding of general relativity (GR) principles
  • Familiarity with cosmic acceleration concepts
  • Knowledge of gravitational growth indices
  • Basic grasp of f(R) gravity models
NEXT STEPS
  • Research the implications of cosmic acceleration on structure formation
  • Study the gravitational growth index γ in various cosmological models
  • Explore f(R) gravity models and their differences from general relativity
  • Investigate the anthropic principle in cosmology
USEFUL FOR

Astronomers, cosmologists, and astrophysicists interested in the dynamics of cosmic structure growth and the implications of cosmic acceleration on the universe's evolution.

wolram
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Why do we live in such a privileged time?

arXiv:1810.10547 [pdf, ps, other]
The End of Cosmic Growth
Eric V. Linder, David Polarski
Comments: 5 pages, 6 figures
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO)

The growth of large scale structure is a battle between gravitational attraction and cosmic acceleration. We investigate the future behavior of cosmic growth under both general relativity (GR) and modified gravity during prolonged acceleration, deriving analytic asymptotic behaviors and showing that gravity generally loses and growth ends. We also note the `why now' problem is equally striking when viewed in terms of the shut down of growth. For many models inside GR the gravitational growth index γ also shows today as a unique time between constant behavior in the past and a higher asymptotic value in the future. Interestingly, while f(R) models depart in this respect dramatically from GR today and in the recent past, their growth indices are identical in the asymptotic future and past.
 
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I think that the title of this thread is misleading the article

wolram said:
arXiv:1810.10547 [pdf, ps, other]
The End of Cosmic Growth
Eric V. Linder, David Polarski
Comments: 5 pages, 6 figures
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO)

is not about the of expansion of the universe, it is about the end of growth of structures in the universe. Very roughly, the proper distance between structures is accelerating, not slowing down, but growth rate of the structures themselves will slow down (in many models).
 
wolram said:
Why do we live in such a privileged time?

There may be a more satisfying answer than the anthropic principle, but that certainly applies. You definitely won't catch fish if your cast doesn't land in water.
 

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