Understanding Accelerating Expansion: Exploring Space Interjection and Density

In summary: So it could be that space is expanding, it could be that space is contracting, it could be that space is changing in some other way, but we would not be able to say anything about it uniquely from GR. That's why I say it's a generalization, and I don't think anyone really knows for sure.
  • #1
keepit
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I'd like to understand accelerating expansion better. It seems that space is interjected proportionately where there is low density (intercalated is the term in biology). Can this interjection of space be sent back where it came from when that area of space becomes more densely populated?
 
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  • #2
To my knowledge the expansion of space is the same everywhere and the density of mass/matter has no effect on it.
 
  • #3
As i understand it, there is no expansion within galaxies where there is much mass.
 
  • #4
keepit said:
As i understand it, there is no expansion within galaxies where there is much mass.

That is incorrect. The force of gravity holds everything together against the expansion. It is only when you get to a scale of galaxy clusters that the effect of expansion starts to overcome gravity. Meaning that cluster A gravitationally attracts cluster B, however the enormous distances between the clusters means that the rate of expansion is starting to overpower gravity, resulting in cluster A and B NOT coming closer together, but getting further apart.
 
  • #5
I'm not sure I'd put it that way, it sounds like a rather Newtonian description of gravity. I get the sense the OP is framed in the language of general relativity with a cosmological constant, in which case it's all gravity-- expansion is gravity, acceleration is gravity, bound orbits in galaxies is gravity. So the way I would put it is, gravity has many aspects, and the local density of matter controls which aspect is most important. On the galaxy scale and smaller, what matters is the gravity of the local masses, and you get bound orbits and no expansion of space (indeed, it is useful to imagine that space is contracting in such environments, though of course this really refers to a particular choice of spatial coordinates). On the scale of the universe as a whole, you have the cosmological principle, and that combines the gravity from the average density over the whole universe (most important for about the first half of the universe expansion) and the gravity from vacuum itself (say in a cosmological constant way, most important for the about the latter half of the expansion). Another crucial factor is the initial condition in time-- we have an expanding universe whenever we "start the clock" of our gravity analysis, and that is yet another aspect of the process we must take into account. So in effect we have an initial condition that is responsible for space being added (which was most important early on, say after inflation), we have dark energy that is responsible for space being added (which is more important recently), we have global mass density that is responsible for space being removed (important early), and we have local galaxies that are responsible for space being removed (important locally only).
 
  • #6
Well, all I can say is that your explanation is one that has never been explained to me. I've always seen it explained the way I did.
 
  • #7
The point is, we should choose a consistent ontology when we talk about what is happening. If we are going to use GR as our model of gravity to say what is happening on cosmological scales, it's quite awkward to use Newton's gravity to say what is going on in galaxies, which is what you are doing (and yes, it is often done I agree). It's not wrong, because GR works for cosmology and Newton works for galaxies, but it's kind of awful to mix the models and use language like "this is what is happening." I feel if one will do that, they should at least say "using a GR model for cosmological gravity, but Newton's model for galactic gravity"..., then everything would be clear (including the nature of the inconsistency). Otherwise, people tend to take explanations too literally, and cannot see the arbitrary choices that are being made in the language. Maybe that much clarity is itself a cause of some issues, but at least they are educational issues.
 
  • #8
So...are you saying that in GR space is not being created inside of galaxies? I've never gotten into the math and details of the expansion of space, but everything I have read has said that space is expanding. I can easily see that this is a generalization and that it could be that space is not expanding if you have sufficient mass in an area of space.
 
  • #9
Drakkith said:
So...are you saying that in GR space is not being created inside of galaxies?
Sorry I missed this for awhile. GR does not provide any unique or observable way to talk about what space is doing, only the curvature of spacetime. There are coordinates we can choose that suggest various things that "space is doing", but they are only pictorial in GR-- they're not unique descriptions of what is happening. I would say that the most natural types of coordinates I can think of would have space being contracted within galaxies (by the galactic gravity) and expanded between clusters of galaxies (by the cosmological solution). If gravity can do one, it can do the other also, and mixing the gravity-as-spacetime-manifold on the cosmic scale with gravity-as-Newtonian-force on the galactic scale seems like mixing apples and oranges, though it does not give a wrong answer.
I've never gotten into the math and details of the expansion of space, but everything I have read has said that space is expanding. I can easily see that this is a generalization and that it could be that space is not expanding if you have sufficient mass in an area of space.
Yes, it seems to me that if we talk about "what space is doing", what we really mean is "what observers are doing who are both inertial and in some sense generic." Inside a galaxy, the natural thing for generic inertial observers to do is fall together, into the core of the galaxy. Outside galaxy clusters, the natural thing for generic inertial observers to do is to drift farther away from each other.
 
  • #10
Wait, are you saying that this "expansion" is just something like reverse curvature? So the curvature is a certain way when mass is present, and the cosmological constant causing a reverse curvature or something similar? I've understood the curvature from mass as causing such effects as light curving around a massive object. How does this effect the travel of light on a universal scale if the curvature is it's the same thing but reversed?
 
  • #11
I have been reading that with the end of the Luminiferous Aether theory that Space itself is truly empty and unlike ponderable matter has no Physical characterisitics at all. Does it therefore make sense to say that space expands to explain how some distant matter is moving away from us at light speed or more? If this expansion at certain distances and attraction locally is all just related to gravity could gravity therefore somehow have a negative sign at large distances?
 
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  • #12
Drakkith, keep in mind that the FRW solution of an isotropically and uniformly expanding spacetime results from an isotropic and uniform energy density as a source. This is really only true on cosmological scales. Locally, on the scale of a galaxy for example, one should expect different gravitational dynamics on account of the inhomogeneous energy density.
 
  • #13
bapowell said:
Drakkith, keep in mind that the FRW solution of an isotropically and uniformly expanding spacetime results from an isotropic and uniform energy density as a source. This is really only true on cosmological scales. Locally, on the scale of a galaxy for example, one should expect different gravitational dynamics on account of the inhomogeneous energy density.

FRW solution?
 
  • #15
Tanelorn said:
I have been reading that with the end of the Luminiferous Aether theory that Space itself is truly empty and unlike ponderable matter has no Physical characterisitics at all.
That doesn't seem to be quite true-- empty space may have a "cosmological constant", which is essentially a tendency to expand, of if you prefer, a negative gravitational effect on objects placed far enough apart.
Does it therefore make sense to say that space expands to explain how some distant matter is moving away from us at light speed or more?
Saying that space expands is one way to communicate the idea. All you can really say is that distances increase, the "why" is rather pictorial.
If this expansion at certain distances and attraction locally is all just related to gravity could gravity therefore somehow have a negative sign at large distances?
That is indeed the idea behind a cosmological constant, if that is what is responsible for the apparent acceleration of the expansion.
 

Related to Understanding Accelerating Expansion: Exploring Space Interjection and Density

What causes the accelerating expansion of space?

The current theory for the accelerating expansion of space is dark energy. This is a hypothetical form of energy that is thought to permeate all of space and is causing the expansion to speed up. However, the exact nature and origin of dark energy is still a mystery.

How is the expansion of space measured?

The expansion of space is measured through the study of distant galaxies and their redshift. This is the phenomenon in which light from distant objects appears to be shifted towards the red end of the spectrum. The amount of redshift can be used to calculate the distance of the object and the rate of expansion of space.

What is the role of space interjection in accelerating expansion?

Space interjection, also known as cosmic inflation, is a theory that suggests in the early stages of the universe, space expanded at an exponential rate. This rapid expansion could have set the stage for the current accelerating expansion of space. However, more research is needed to fully understand the relationship between space interjection and accelerating expansion.

How does density affect accelerating expansion?

Density is a key factor in determining the fate of the universe and the rate of its expansion. The current theory suggests that the density of matter and energy in the universe will determine if the expansion will continue to accelerate, eventually slow down, or even reverse. Higher densities are thought to lead to a slower expansion, while lower densities result in a faster expansion.

What are the implications of accelerating expansion for the future of the universe?

The implications of accelerating expansion are still being studied and debated. Some theories suggest that the universe will continue to expand at an ever-increasing rate, causing galaxies to become further apart and eventually leading to the "heat death" of the universe. However, other theories propose that the expansion may eventually slow down or reverse, potentially leading to a "big crunch" scenario. More research is needed to understand the ultimate fate of the universe.

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