Undergrad The Acceleration and the density of galaxies

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SUMMARY

The discussion centers on the implications of the Lambda-CDM model regarding the decreasing density of galaxies as the universe expands. It is established that while the density of galaxies diminishes, it does not completely vanish; rather, the number of visible galaxies decreases due to the accelerated expansion of the universe. The book "A Universe from Nothing" by Lawrence Krauss is referenced for its discussion on this topic, specifically in the chapter titled "Our Miserable Future." Additionally, a paper available at arxiv.org is cited for further clarification on this misconception.

PREREQUISITES
  • Understanding of the Lambda-CDM model in cosmology
  • Familiarity with concepts of cosmic expansion and density
  • Knowledge of observational astronomy and galaxy visibility
  • Basic comprehension of light propagation in an expanding universe
NEXT STEPS
  • Read "A Universe from Nothing" by Lawrence Krauss for insights on cosmic expansion
  • Review the paper at arxiv.org for detailed calculations related to galaxy visibility
  • Explore the implications of the Lambda-CDM model on galaxy formation and distribution
  • Investigate the effects of accelerated expansion on observable universe metrics
USEFUL FOR

Astronomers, cosmologists, and astrophysics students interested in the dynamics of galaxy density and the implications of cosmic expansion will benefit from this discussion.

mbond
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In the Lambda-CDM model, the density of galaxies goes decreasing and should even vanish in the far future.

I would be grateful if someone could point me to a paper where this is calculated.
 
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It is a simple inference from the number of galaxies in a comoving volume staying constant while the size of the comoving volume increases. This just has to do with expansion itself, accelerated expansion is not required.
 
Also, as the universe expands, the density of galaxies decreases, but it never "vanishes".
 
I mean the number of visible galaxies goes vanishing because of the Acceleration. This is told in the book "A universe from nothing" by L.. Krauss, chapter "Our miserable future". Is there a paper or a reference where this is calculated?
 
mbond said:
I mean the number of visible galaxies goes vanishing because of the Acceleration. This is told in the book "A universe from nothing" by L.. Krauss, chapter "Our miserable future". Is there a paper or a reference where this is calculated?
This looks like a common misconception. Objects once seen never disappear. Apart from getting ever dimmer until eventually too hard to observe, that is. But the light is still there, reaching the observer.
Krauss has been guilty of wording this less-than-ideally in at least one other book - see e.g. this paper: https://arxiv.org/abs/astro-ph/0310808, example 13 in appendix B.
 
mbond said:
I mean the number of visible galaxies goes vanishing because of the Acceleration. This is told in the book "A universe from nothing" by L.. Krauss, chapter "Our miserable future". Is there a paper or a reference where this is calculated?
In addition to Bandersnatch's comment, nearby galaxies aren't moving apart. It isn't immediately obvious that they would ever necessarily spread out far enough to be part of the fading Bandersnatch mentions.
 

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