Understanding the Expansion of Space: Galaxies Moving Away and Proving Expansion

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Discussion Overview

The discussion revolves around the concept of the expansion of space, particularly focusing on how the observation that galaxies are moving away from each other supports the idea of space itself expanding rather than galaxies moving through a static space. Participants explore theoretical implications, interpretations of cosmological observations, and the relationship between space and motion.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants propose that the observation of galaxies moving away at rates proportional to their distance is synonymous with the statement "space is expanding."
  • Others argue that the Einstein Field Equations provide a framework for understanding the relationship between the expansion of space and the behavior of galaxies.
  • A question is raised about the implications of being at the "center" of the universe and whether the observed movement of galaxies would differ.
  • Some participants assert that there is no "center" of the universe, and the expansion appears the same from any location, aligning with standard cosmological assumptions.
  • There is a discussion about the redshift/distance relation and its incompatibility with the idea of galaxies moving through space, with some noting that this interpretation can vary based on distance.
  • One participant suggests that from a relativity perspective, the concept of "things moving through space" is problematic, as motion is relative to a frame of reference.
  • Another viewpoint emphasizes that while there is a preferred reference frame in cosmology, it is more accurate to describe it as a convenient frame rather than a "preferred" one.
  • Some participants express confusion over the terminology of "space expanding" versus "distances between objects increasing," noting that both phrases can lead to misconceptions.
  • There is a recognition that both descriptions—expansion of space and increasing distances—are convention-dependent and can be misleading in different contexts.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the interpretation of cosmic expansion, the nature of reference frames, and the implications of terminology used in describing these concepts. The discussion remains unresolved with no consensus on the preferred terminology or interpretation.

Contextual Notes

Limitations include varying interpretations of cosmological observations, dependence on definitions of motion and reference frames, and unresolved nuances in the relationship between space and the movement of galaxies.

  • #61
rede96 said:
Can you define what being in “free fall” means?
If an object is in free fall its trajectory is a 'geodesic'. In this case the object doesn't feel a force acting on it. This is true for Galaxies, planets orbiting around a star and apples falling down to Earth.
 
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  • #62
rede96 said:
I found it a good way to conceptually think of expansion that fits with what we see in observation and has some basis in physics. (E.g. QFT, the FRW equations, inflation theory etc.)

As @timdeeg has pointed out, this does not fit with observation because your model predicts that galaxies should feel a force, and they don't.

The reason the concept of "space expanding" doesn't make sense is that "space" is frame-dependent, and the laws of physics are frame-independent. So whatever is going on in the universe, "space expanding" can't be a good description of it.
 
  • #63
timmdeeg said:
If an object is in free fall its trajectory is a 'geodesic'. In this case the object doesn't feel a force acting on it. This is true for Galaxies, planets orbiting around a star and apples falling down to Earth.

If I understood you correctly your saying that expansion is due to space time curvature. Correct?
 
  • #64
PeterDonis said:
As @timdeeg has pointed out, this does not fit with observation because your model predicts that galaxies should feel a force, and they don't

I was using ‘force’ in very loose terms just to indicate there was something going on to cause objects to move apart. I wasn’t implying they felt any force from acceleration. The way I thought about it wouldn’t be any different.
 
  • #65
rede96 said:
I was using ‘force’ in very loose terms just to indicate there was something going on to cause objects to move apart.

Then you shouldn't use the word "force", because it will only lead to confusion. Not just for others, but for you. It leads you to think that "there was something going on to cause objects to move apart". There isn't. There is just the geometry of spacetime.

To illustrate what I mean, consider tidal gravity: two objects free-falling radially above a gravitating mass (like the Earth), starting from slightly different altitudes. These objects will move apart as they fall. Is there "something going on" that causes this? If so, what is this "something"? If not, how is this case different from the expansion of the universe?
 
  • #66
rede96 said:
If I understood you correctly your saying that expansion is due to space time curvature. Correct?
Well, to know what geodesic means is not the clue to have a notion of what expansion means. But you can imagine two neighboring geodesics describing the trajectories of two objects. If the spacetime is curved then their geodesics accelerate relative to each other, in the case of an expanding universe they accelerate away from each other. Whereas if the spacetime is flat their relative acceleration is zero (which doesn't exclude of course that these particles move relative to each other with constant speed).
 
  • #67
timmdeeg said:
If the spacetime is curved then their geodesics accelerate relative to each other, in the case of an expanding universe they accelerate away from each other.

This is not quite right. In a matter-dominated universe the expansion is decelerating, and the geodesics in question (the worldlines of comoving objects) are converging, not diverging. But the universe is still expanding.

The correct definition of "expanding" for the universe is that the congruence of worldlines of comoving objects has a positive expansion scalar. Unfortunately, that's already getting beyond the "B" level of this thread. But you can find more information here:

https://en.wikipedia.org/wiki/Congr...atical_decomposition_of_a_timelike_congruence
 
  • #68
rede96 said:
your saying that expansion is due to space time curvature.

The expansion is due to the positive expansion scalar of the congruence of comoving worldlines (see my previous post). But the fact that such a congruence exists and has the properties it has (not just positive expansion, but every comoving observer sees the universe as homogeneous and isotropic) is due to the particular geometry of the spacetime in question (FRW spacetime).
 
  • #69
PeterDonis said:
This is not quite right. In a matter-dominated universe the expansion is decelerating, and the geodesics in question (the worldlines of comoving objects) are converging, not diverging. But the universe is still expanding.
Ah yes, it follows from the second Friedmann equation that the second derivative of the scale factor is negative in this case (what I didn’t take into account). Thanks for correcting and for the link.
 
  • #70
This is an old thread but my understanding is that there is an idea from quantum physics that says that empty space may be teeming with activity at a quantum level. I thought this might be of interest to the OP if he is still around.
 
  • #71
Dan White said:
This is an old thread but my understanding is that there is an idea from quantum physics that says that empty space may be teeming with activity at a quantum level.
This appears in our current cosmological model as dark energy. We don't fully understand why its density is so small (about 120 orders of magnitude smaller than the value that the basic quantum physics calculation you refer to gives), but it is there in the model.
 
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  • #72
PeterDonis said:
This appears in our current cosmological model as dark energy. We don't fully understand why its density is so small (about 120 orders of magnitude smaller than the value that the basic quantum physics calculation you refer to gives), but it is there in the model.
I think that is taking things for granted a bit too far. In the cosmological model the cosmological constant is just a parameter without any particular origin. In the quantum zero point energy could theoretically contribute to this but is, as you say, 120 orders of magnitude off which if anything is an indication that the connection to the cosmological constant is not well understood. Ideally a theory of quantum gravity should of course address this.
 
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  • #73
Orodruin said:
In the cosmological model the cosmological constant is just a parameter without any particular origin.
True, but any "activity of empty space" of the sort the poster I responded to was describing would have to appear in our cosmological model in this parameter. So our cosmological model already takes into account the possibility that such a thing exists. The value we use in our model is based on empirical observation and we don't have a good theoretical understanding of why that is the value we observe, but that doesn't mean our model doesn't take the possibility into account.
 
  • #74
Orodruin said:
I think that is taking things for granted a bit too far. In the cosmological model the cosmological constant is just a parameter without any particular origin. In the quantum zero point energy could theoretically contribute to this but is, as you say, 120 orders of magnitude off which if anything is an indication that the connection to the cosmological constant is not well understood. Ideally a theory of quantum gravity should of course address this.
Well, in principle our Standard Model of HEP doesn't tell us at all what the absolute value of the vacuum energy (density) is. In the usual perturbative treatment it's set to 0 by imposing "normal ordering" or equivalently by renormalization of the vacuum diagrams. This introduces a renormalization scale, and when using the renormalization group to go from the low-energy scale to very high scales (GUT scale or even the Planck scale) you get these huge 120 orders of magnitude discrepancies.

I think in this sense the vacuum-energy/cosmological-constant problem is the least understood "today observable part" on the crossroad between GR and QT. Maybe it's solved one day when a consistent formulation of "quantum gravity" is found.
 
  • #75
vanhees71 said:
I think in this sense the vacuum-energy/cosmological-constant problem is the least understood "today observable part" on the crossroad between GR and QT.
Do we have at least a hint why it acts as "repelling" gravity?
 
  • #76
timmdeeg said:
Do we have at least a hint why it acts as "repelling" gravity?
We have more than a hint. What you are calling "repelling gravity" is what the Einstein Field Equation says you get when you have the stress-energy of a perfect fluid with an equation of state ##p = - \rho##. And that's exactly what you have with a cosmological constant.
 
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  • #77
PeterDonis said:
We have more than a hint. What you are calling "repelling gravity" is what the Einstein Field Equation says you get when you have the stress-energy of a perfect fluid with an equation of state ##p = - \rho##. And that's exactly what you have with a cosmological constant.
Thanks. I have another question in this context.

The value of the Cosmological Constant according to the Quantum Field Theory is much to high. But apart from this it's sign due to QFT seems correct. In other words QFT having no link to General Relativity doesn't just predict a vacuum energy density, it predicts the vacuum energy density with the correct sign to act like the CC. Is that correct?
 
  • #78
timmdeeg said:
QFT having no link to General Relativity doesn't just predict a vacuum energy density, it predicts the vacuum energy density with the correct sign to act like the CC. Is that correct?
AFAIK yes, QFT predicts a positive sign for the vacuum energy density.
 
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  • #79
Space without matter still has fields: electromagnetic field, gravitational field, Higgs field, etc. It also has energy, so "empty" space isn't nothing.
 

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