How seriously do you take the FLRW model?

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Discussion Overview

The discussion centers around the FLRW (Friedmann-Lemaître-Robertson-Walker) model of cosmology, particularly its assumptions of isotropy and homogeneity, and the implications of hypothetical alterations to the universe's density and curvature. Participants explore theoretical scenarios and thought experiments related to the model's validity and physical implications.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification
  • Mathematical reasoning

Main Points Raised

  • Some participants note that the scale of homogeneity in the universe seems to shift as larger structures are observed, suggesting a moving target for defining homogeneity.
  • One participant proposes a thought experiment where removing hydrogen atoms from the universe could lead to different curvature scenarios, raising questions about the relationship between density and curvature.
  • Another participant argues that the curvature of the universe would remain unchanged despite alterations in density, asserting that it is the rate of expansion that would be affected.
  • Some participants discuss the implications of altering density on the critical density and the potential contradictions that arise from such changes.
  • There is a mention of the conservation of the stress-energy tensor and how violating this principle would lead to ambiguous results in the context of the FLRW model.
  • One participant emphasizes the importance of grounding discussions in mainstream physics while acknowledging the value of exploring toy examples for understanding concepts.
  • Several participants engage in a debate about the nature of inhabited parts of the universe, with differing views on whether all inhabited regions are finite or if the universe can be infinite beyond observable limits.
  • There are discussions about the implications of dark matter and dark energy in cosmology, with some participants expressing skepticism about the current understanding of these concepts.

Areas of Agreement / Disagreement

Participants express a range of views, with no clear consensus on the implications of the thought experiment or the nature of the universe's curvature and density. Disagreements arise regarding the relationship between density changes and curvature, as well as the interpretation of inhabited regions of the universe.

Contextual Notes

The discussion involves speculative scenarios that challenge the assumptions of the FLRW model, with participants acknowledging the unphysical nature of some thought experiments. Limitations in the assumptions made and the dependence on definitions are noted but remain unresolved.

skippy1729
1. Isotropic? yes.

2. Homogeneous? Historically, the scale of homogeneity seems to be a moving target. As ever larger structures are observed, the scale of homogeneity is set just past the horizon, so to speak.

My real problem comes from the following thought experiment. Actually a pseudo thought experiment since it can not be performed.

Suppose the universe has a slight positive curvature. It is then closed and contains a finite amount of stuff. Now, by magic, we take one hydrogen atom from every cubic kilometer and make it disappear.
The curvature could now be exactly zero, or slightly negative. There are now two alternatives:

A. The universe could spontaneously transmute into an infinite flat or hyperbolic space containing an infinite amount of stuff.

B. The universe could spontaneously transmute into a flat toroidal or closed hyperbolic space, still with a finite amount of stuff.

My (scientifically unjustified) opinion of this pseudo experiment is that the universe should be finite. Perhaps I am just taking the model too seriously.

Cheers, Skippy
 
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The curvature would be unchanged. I think it is the rate of expansion that would alter.
 
Skippy, I like your thought experiment.
skippy1729 said:
... Now, by magic, we take one hydrogen atom from every cubic kilometer and make it disappear.
The curvature could now be exactly zero, or slightly negative. There are now two alternatives:
...

However I agree with Sylas.

sylas said:
The curvature would be unchanged. I think it is the rate of expansion that would alter.

Of course the thought experiment involves magic so it is somewhat unphysical. But to spell it out in more detail let's recall that the critical (energy) density is

rhocrit = 3 c^2 H^2/(8 pi G)

Now in your example you start with slight positive curved spatial closed universe (topologically a bumpy hypersphere)

say rho = 1.01 rhocrit = 3.03 c^2 H^2/(8 pi G) where H is the Hubble (expansion) rate, G is Newton, and c is c.

Now you reduce rho, say by 1 percent.

If H would stay the same, then you have a contradiction because now rho would equal rho_crit and she should be spatial flat infinite. That is your paradox. But maybe at the same time H decreases (by magic too). So that rho_crit reduces, say also by 1 percent. then you have the same old positive curved situation with your new density!

Again rho = 1.01 rhocrit and it is the same old hypersphere as before.
 
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Thanks, I should have realized that magically changing rho would also magically change H, keeping everything (sort of) the same.

Skippy
 
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skippy1729 said:
Thanks, I should have realized that magically changing rho would also magically change H, keeping everything (sort of) the same.

Skippy

Heh heh. Well there is so much magic involved that it is hard to say how any of it could be physically implemented, so it is hard to say honestly what would actually happen. But I think it is an instructive question to ask, and hope you keep probing like that.
 
Chronos said:
Read mainstream papers is my recommedation. Opinions do not cut it.

I don't think a mainstream paper will really deal with this thought experiment, which is pretty unphysical as phrased. But if you have a reference, that's fine.

Surely there is some value in trying to apply ones own knowledge of mainstream physics to toy examples. Otherwise why have a forum at all? We could all just sit back and read mainstream papers.

In my experience, I learn by reading and then applying -- and being corrected by others when I go wrong.

In this case, I suspect skippy is thinking in terms of simple equations like
[tex] \left(\frac{a}{\dot{a}}\right)^2 + \frac{kc^2}{a^2} - \frac{\Lambda c^2}{3} = \frac{8 \pi G}{3} \rho[/tex]​

He's presumed that altering density (rho) would require an alteration to curvature. My point is simply that there's the [itex]\dot{a}[/itex] term he appears to have missed. Altering the energy density will alter the rate of expansion (and hence the rate of change of curvature), rather than altering curvature.

Cheers -- sylas
 
Well, considering that such an alteration of the density would violate conservation of the stress-energy tensor, a law upon which the FLRW expansion is based, the result would be ambiguous.
 
Apologies for the incomplete post. One of my favorite presentations is by Sean Carroll:
http://preposterousuniverse.com/writings/cosmologyprimer/index.html
 
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The inhabited parts of the universe are finite -- the rest can be anything you want it to be.
 
  • #10
Hal King said:
The inhabited parts of the universe are finite
Why? How do you know?

Hal King said:
the rest can be anything you want it to be.
I don't think reality cares what we want.
 
  • #11
I'm assuming we occupy a typical 'inhabited' part and we can only see a finite amount of universe.
(If we don't occupy an inhabited part, I'm not sure where that leads us.)

And 'reality' doesn't effect the unknowable. You can make up whatever you want with no fear of being proved wrong.

But I guess, this thread started by evoking 'magic' .. so anything is possible.
 
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  • #12
Hal King said:
I'm assuming we occupy a typical 'inhabited' part and we can only see a finite amount of universe.
(If we don't occupy an inhabited part, I'm not sure where that leads us.)
Well, perhaps if you meant that each individual inhabited part is finite, then you're okay. But it sounded like you meant that all inhabited parts in total are finite, which is by no means known.

Hal King said:
And 'reality' doesn't effect the unknowable. You can make up whatever you want with no fear of being proved wrong.

But I guess, this thread started by evoking 'magic' .. so anything is possible.
Failure to be proven wrong doesn't mean you aren't. So it's better to ask what is likely to be correct, instead of what insane nonsense can I make up that can never be tested.
 
  • #13
I do agree with that ... but what does that mean for much cosmology today?
 
  • #14
Hal King said:
I do agree with that ... but what does that mean for much cosmology today?
Nothing, because cosmology is an observation-driven science.
 
  • #15
Or better a science driven by what can't been seen ... dark matter, dark energy, ... ?
 
  • #16
Hal King said:
Or better a science driven by what can't been seen ... dark matter, dark energy, ... ?
That is more than a little facile.
 
  • #17
Better than a 'rub goldberg' one.
 

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