Does Space Expand? What Do You Think?

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The discussion centers on the interpretation of the universe's expansion, questioning whether space itself is expanding or if it's merely a kinematic effect. Cosmologists often describe redshifts as a result of expanding space, but some, including John Peacock, argue that this interpretation can be misleading. The conversation highlights a thought experiment involving a galaxy held stationary in an expanding universe, illustrating that its behavior contradicts the common understanding of expansion. Participants suggest that focusing on increasing distances rather than expanding space might clarify misconceptions. Ultimately, the debate reflects ongoing discussions about the nature of distance and expansion in general relativity.
  • #51
I'm also interested in the expert opinions.
My understanding may need some revising.
Since the speed of light is constant, (unit of distance/unit of time) then the ratio always has to 1/1, 2/2, etc. otherwise there would be a change in the speed of light.
In order to keep the speed of light constant both the distant units and the time units have to change at the same moment.
Has this been observed? What changes would we observe? Only Red shift?
I'll listen.
jal
 
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  • #52
In this discussion AFAIK nobody is talking about the UNITS of time or distance changing, Jal.

distances between utterly separate disconnected things change, and they change as measured by units which are assumed to be constant and reliable

the cosmological redshift epitomizes a process which for better or for worse has always been described as the expansion of space

==============

If anyone is familiar with what Galileo is supposed to have said or muttered:
Eppur' si muove.

it could be adapted to modern context:
Eppur' si 'spanda.

In spoken Italian a lot of syllables get dropped, if you want to use babelfish to translate you have to write the words out
Eppure si espanda.
 
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  • #53
marcus said:
But I am not comfortable with that because among other things I see cosmologists doing inventories of the energy density which are implicitly estimated IN A CMB FRAME... (etc)

This and the rest of that post isn't wrong, we can and do define things wrt to the CMB 'rest' frame and the energy of the CMB photons does decline with the fourth power of the scale factor. The interpretation that they do this by traveling through some stretching stuff we call space is this issue. How many time have you seen a demo where someone draws a wave on a balloon then blows it up? The problem with thinking of expanding space like this is that implies the expansion acts like a viscous force, dragging photons and galaxies apart.

My view on galaxies and expanding space has, I think, been explained already in this thread. For photons I do think it is better to think of them as being redshifted by being observed in a different frame. However, to be clear what a mean by this, consider the FRW metric for a flat universe:

d\tau^2 = -dt^2 + a(t)[dr^2 + d\Omega^2]

Now at t ticks along, the scale factor a(t) increases. Therefore two observers who are both at rest wrt to the CMB, but who have different times t will therefore be in different frames (have different metrics). This is what leads to photons being redshifted when observed and emitted at different times.
 
  • #54
marcus said:
Hi jal,

from the standpoint of an observer at rest wrt CMB
an electromagnetic wave has its wavelength enlarged in accordance with the scalefactor a(t)[/color]
and this process goes on constantly as the wave travels thru the universe.

\frac{\lambda_t}{\lambda_{emitted}} = \frac{a(t)}{a(t_{emitted})}

if you know the wavelength when the wave was emitted and you know the ratio by which the universe has expanded since the time when it was emitted---that is the ratio on the righthand side---then you know the wave's wavelength at any given time.

(everything is always understood to be seen from the standpoint of an observer at rest wrt Hubble flow)

Now I have to see if that is compatible or not with what the experts say.

This relationship can be derived without any notion of "stretchy space", given that one assumes that the universe has a FRW metric. The FRW metric can be derived assuming the universe is isotropic, and that GR is valid.

If you have MTW's "Gravitation", see for instance 29.10 on pg 778.

The basic approach is simply to solve for the geodesics of light. Assuming all the motion is in the radial direction

-dt^2 + a(t)^2 dr^2 = 0 implies that dt = a(t) dr, or

r(t) = \int \frac{dt}{a(t)}

The rest is just algebra.
 
  • #55
I am totally on board with Wallace on this issue. My hangup is my inability to mathematically describe our observable universe without at least one more degree of freedom. I vaguely recall a similar problem with too few degrees of freedom that predicts the energy potential of empty space is absurdly large. Is this a modern day 'ultraviolet catastrophe'?
 
  • #56
Wallace said:
How many time have you seen a demo where someone draws a wave on a balloon then blows it up? The problem with thinking of expanding space ...

Let me point out that the reason for much confusion is that the familiar word "expansion" has connotations which have nothing to do with changing metrics --- which are of the essence in your thread, Wallace.

In practical ordinary life, e.g. in introductory physics, "expansion", say of a heated rod, is measured relative to a practical invariant standard, say an invar measuring tape. Our familiarity with such a typical use of the word "expansion" has unfortunately come to colour our thinking about cosmology.

In cosmology, "expansion", refers to something altogether more strange and unfamiliar to practical ordinary life: a change in a metric coefficient a(t) in the expression:

the FRW metric for a flat universe:

d\tau^2 = -dt^2 + a(t)[dr^2 + d\Omega^2]

"Expansion", used to describe this change, is shorthand for "the effect produced by that change in the ratio of the metric coefficients of the FRW metric that leaves physics invariant". We have no everyday word for such a change. But the historically natural choice of "expansion" as shorthand for this phrase has turned out to be unfortunate. It produces much confusion about "expanding space".

Also, it seems, there are confusions about what happens to photons as they travel between emission and absorption (as expressed in this thread by Marcus). The correct view of redshift is, as you have explained, Wallace:

I do think it is better to think of (photons) as being redshifted by being observed in a different frame ...Now at t ticks along, the scale factor a(t) increases. Therefore two observers who are both at rest wrt to the CMB, but who have different times t will therefore be in different frames (have different metrics). This is what leads to photons being redshifted when observed and emitted at different times.

I guess it's far too late now to invent a new word to describe the changes in the metric of spacetime that cosmologists have uncovered. They will just have live with the semantic confusions about expansion that they have inherited.
 
  • #57
P.s.

Wallace said:
two observers who are both at rest wrt to the CMB, but who have different times t will therefore be in different frames (have different metrics). This is what leads to photons being redshifted when observed and emitted at different times.

I agree fully with what you say here, Wallace, as I said in my previous post. This post is to unpack some implications of what you said.

It is that the observers and the photons that are emitted or absorbed (all of which are very localised, in our case deep inside a gravitationally bound galaxy) will have as their local metric the FRW metric of the universe that prevails at the time of emission or absorption.

This means that at a particular instant of universal time the FRW metric of the universe prevails on all scales and everywhere, even inside gravitationally bound structures or within atoms. And that using it with the appropriate scale factor will always yield the same physics. The only caveat is that this metric, which changes dramatically over times comparable with the age of the universe, may be perturbed by local mass concentrations. In a laboratory or observatory these perturbations are hopefully not large enough to perceptibly affect spectral light.

Using the word "expansion" to describe what is going on in the universe doesn't sit well with this situation. Something like "Universal rescaling" might fit better.
 
  • #58
oldman said:
In cosmology it is obvious that talking of "expanding space" , as if space was an elastic continuum is just plain silly. For instance, Matter --- crystals, atoms, nuclei and suchlike --- are mostly empty "space", as is the dispersion of galaxies that constitutes the universe. If you describe change in the universe as the expansion of "space" you are then faced with the difficulty of
distinguishing between two sorts of "space", non-expanding "space" in microscopic interstices and inter-galactic- cluster “ expanding space”.
You alluded to other difficulties but did not specify them so they may be cogent, I can't say. Furthermore, I am not an expert in GR so the following comments may be subject to correction. However, I don't see this "two sorts of space" as a difficulty at all. IF you accept the "expanding space" view, THEN: Within an atom, the particles are bound by forces as strong as the chain mentioned in post #3 in this thread. As space expands, it oozes right out of the atom like bread rising around raisins that are held fixed by chains.
 
  • #59
jimmysnyder said:
...I don't see this "two sorts of space" as a difficulty at all. IF you accept the "expanding space" view, THEN: Within an atom, the particles are bound by forces as strong as the chain mentioned in post #3 in this thread. As space expands, it oozes right out of the atom like bread rising around raisins that are held fixed by chains.

I agree with your IF...THEN; there is always a way of resolving problems by exercizing one's imagination. The as-yet unexplored rheology of "space" may yet come to be of interest to cosmologists! Thanks for the comment.
 
  • #60
oldman said:
This means that at a particular instant of universal time the FRW metric of the universe prevails on all scales and everywhere, even inside gravitationally bound structures or within atoms. And that using it with the appropriate scale factor will always yield the same physics. The only caveat is that this metric, which changes dramatically over times comparable with the age of the universe, may be perturbed by local mass concentrations. In a laboratory or observatory these perturbations are hopefully not large enough to perceptibly affect spectral light.

Ouch! I have to step in a disagree with you here oldman (I permit you to ignore me as a young whipper snapper if you wish :biggrin: ). The FRW metric, and the 'expansion' (I agree that's an awful word to describe the effect) does not have an effect on small scales in our universe. Local mass concentrations are far more than merely a perturbation to FRW on familiar scales. If anything there is a vanishingly small FRW element to the metric of bound structures.

If the FRW metric 'prevail(ed) on all scales and everywhere, even inside gravitationally bound structures or within atoms' then why do galaxies maintain a constant size as the distance between them expands? Commonly we are told that the local mass concentration 'overcomes' the expansion preventing this from occurring. This is one of the worst and most fallacious explanations you could possibly give someone! What really happens then?

The FRW metric is the inevitable result of the cosmological principle, which is that the universe is homogeneous and isotropic. The metric is only valid if these principles hold. Consider now a galaxy, solar system or planet. Does the CP hold? No. Is it a remotely useful approximation? Not at all! Unsurprisingly then the dynamics of bodies in these systems and on these scales bears no resemblance to the dynamics of galaxies. So for instance, there is no redshift of light due to a(t) when we observe light from the other side of our galaxy, or from say Andromeda. The FRW metric simply is not valid on these scales.

Remember that there is no force due to gravity. However when we say that a galaxies mass 'overcomes' the expansion we on the one hand mistreat the expansion of the universe as acting as some kind of viscous force then on the other hand treat the galaxy self gravity as a force overcoming this global effect. This is a horrible hodjpog situation. The better way to look at it is that the presence of the mass in the galaxy gives the metric of space-time around this mass a form that would look much more like a Schwarzschild metric than FRW (though we cannot fully solve GR for a galaxy..). The point is though that there is not expansion to 'overcome' since the 'expansion' is merely the result of the metric formed by a homogeneous and isotropic mass distribution. If the mass dosn't obey these principles we shouldn't be surprised that we don't see any 'expansion'.

If you don't believe me hold an object in each hand with outstretched arms. When you let them go what happens? I think you will find that they both plummet towards the local centre of mass (the centre of the Earth) rather than drift off into the Hubble flow! The local mass concentration can hardly be described as a mere perturbation to the FRW metric!

Sorry for all the !'s I get rather excited when I talk about this stuff :redface:
 
  • #61
Wallace said:
Commonly we are told that the local mass concentration 'overcomes' the expansion preventing this from occurring. This is one of the worst and most fallacious explanations you could possibly give someone!
I could not agree more on this.

Wallace said:
Sorry for all the !'s I get rather excited when I talk about this stuff :redface:
Well, keep talking about it! :smile:

By the way an excellent explanation Wallace!
 
  • #62
Wallace said:
The FRW metric, and the 'expansion' does not have an effect on small scales in our universe. Local mass concentrations are far more than merely a perturbation to FRW on familiar scales. If anything there is a vanishingly small FRW element to the metric of bound structures.

I guess our disagreements are more a case of crossed wires (due to my careless writing about gravitationally bound structures) than a disagreement. At least I hope so!

I see it like this:

First, consider a classic dust-filled fluid-like universe described by the FRW metric, but filled with CMB radiation (no structures). Let all dust particles be at rest in their local CMB frames (no peculiar motions). The Cosmological Principle rules strictly here. Yet the proper separations of dust particles vary as a(t) changes with time! Strange but true! This is GR, remember ... not simple expansion.


In bound structures with finite volumes cohesion (due to any kind of nature's interactions ... gravitational, electroweak or strong) endows individual components of the structure with kinematic or coasting velocities relative to local CMB frames. These velocities can ensure that proper distances between components remain constant while H remains constant. (Please don't ask me what happens in an inflating, accelerating or decelerating universe!). Ask Pervect!

Thus, in a gravitationally bound galaxy, stars on opposite sides have coasting velocities relative to their local CMB frames. And, atoms in a molecule in deep space have (very, very, very tiny) velocities relative to their local CMB frames.

This is how, as you say:

galaxies maintain a constant size as the distance between them expands?

while the FRW metric nevertheless "prevails" everywhere (a poor word choice of mine, I'm afraid). I should have said "applies but imperceptibly in cases of practical interest". Perturbation was also the wrong word to use.

But then I could accuse you of my own sin, when you say:
The FRW metric simply is not valid on these scales.

valid?
 
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  • #63
I think we pretty much agree on clarification and reflection. I just think it's important to be clear that the 'expansion' (which we both definitely agree is a bad term for it!) is a result of the FRW metric, in particular a(t). The metric in the region of bound structure looks nothing like the FRW metric, in particular it has no global time dependence (though will of course evolve). For this reason I stand by the statement that the FRW metric is not valid on scales which are significantly inhomogeneous, since the metric has no component that reflects the global a(t), and hence the FRW picture does not relate to the dynamics of the system.
 
  • #64
I can't refrain from pointing out that during inflation, where H increases exponentially (if I remember correctly), even the tiniest structures experience a huge disruptive force as a result of the rule of the FRW metric. Pervect convinced me that these forces are vast enough to tear apart just about any structure we can imagine. Yet nobody seems to take notice of this extreme effect! Strange.
 
  • #65
Isn't it possible that close galactic clumps currently receding could in a matter of say 10 billion years, be seen as a part of a larger system, by which anyone of them could have a blue shift from our vantage point? This is something tantamount to the universe evolving, wherein our current universal state of evolution is that of clumps of galaxies held together by gravity, and a later state of evolution we will see clusters of clumps held together by gravity, and further down the line ... clumps of clusters held together by gravity?

It would seem realistic to assume that earlier on in the history of the universe, that all galaxies were seen to be receding from our vantage point, and much earlier than that, matter the size of a standard average every day sun would see all suns receding from the vantage point of every sun. Taken much earlier - all atoms are seen from the vantage point of any atom to be receding.

If this is so, then the idea of space expanding seems frivolous. An accelerated expansion even more so.
 
  • #66
Castlegate said:
Isn't it possible that close galactic clumps currently receding could in a matter of say 10 billion years, be seen as a part of a larger system, by which anyone of them could have a blue shift from our vantage point? This is something tantamount to the universe evolving, wherein our current universal state of evolution is that of clumps of galaxies held together by gravity, and a later state of evolution we will see clusters of clumps held together by gravity, and further down the line ... clumps of clusters held together by gravity?

It would seem realistic to assume that earlier on in the history of the universe, that all galaxies were seen to be receding from our vantage point, and much earlier than that, matter the size of a standard average every day sun would see all suns receding from the vantage point of every sun. Taken much earlier - all atoms are seen from the vantage point of any atom to be receding.

If this is so, then the idea of space expanding seems frivolous. An accelerated expansion even more so.

I'm not quite sure what your point is. A hypothetical universe where everything was inititally redshifting, continuously evolving towards less and less redshift, then started to blueshift is imaginable. Furthermore, it is imaginablie in the context of GR - such a universe would have a matter density over the critical, and would be a universe ending in a "big crunch".

However, experimental data does not support this. As is widely known, the universal expansion appears to be accelerating.

I don't understand why you think the experimental data that says that the universe is expanding and that the expansion is accelerating is "frivolous".

The redshift data is pretty clear evidence that the universe is currently expanding. Even more convincing is that fact that distant supernovae explosions appear to happen "in slow motion" due to time dilation - this basically rules out "tired light" type theories. So for starters, I hope we can agree that the universe is currently expanding.

It does require GR to go beyond saying that the universe is currently expanding to interpret the data as saying that the expansion is accelerating and will continue to accelerate. It is possible using some non-GR theories ,to have a non-accelerating expansion that fits the data. AFAIK there isn't any alternative theory "in play" that suggests that the expansion could reverse, however.

Basically, GR isn't "frivolous" - it's being tested even as we speak. One of the simplest forms of the alternative gravitational theories that would allow non-accelerating expansion has recently been ruled out by the Gravity probe B experiments, for instance. Other more complex forms of this theory may still be viable, but GR has a long history of making good, correct predictions.
 
  • #67
oldman said:
I can't refrain from pointing out that during inflation, where H increases exponentially (if I remember correctly), even the tiniest structures experience a huge disruptive force as a result of the rule of the FRW metric. Pervect convinced me that these forces are vast enough to tear apart just about any structure we can imagine. Yet nobody seems to take notice of this extreme effect! Strange.

I think that the people concerned with large scale structure have to take this effect into account - but they don't tend to popularize their work in such simple terms.

There is a rather subtle point here - when one looks at the actual tidal forces generated by the Riemann, it is not the expansion of the universe that causes these forces, but the acceleration of the expansion of the universe. This is a point that's been discussed before, but I'm too lazy to look up the threads unless there is some renewed interest. Basically, if one considers a universe with no cosmological constant and no "dark energy", there could never be "tearing apart" tidal forces, there could only be compressive tidal forces.

Of course, inflation has effectively an extremely large cosmological constant - and this is what causes the "tearing apart" forces in the usual inflationary schenario.
 
  • #68
Wallace said:
I think we pretty much agree on clarification and reflection. I just think it's important to be clear that the 'expansion' (which we both definitely agree is a bad term for it!) is a result of the FRW metric, in particular a(t). The metric in the region of bound structure looks nothing like the FRW metric, in particular it has no global time dependence (though will of course evolve). For this reason I stand by the statement that the FRW metric is not valid on scales which are significantly inhomogeneous, since the metric has no component that reflects the global a(t), and hence the FRW picture does not relate to the dynamics of the system.


While it may not make sense to use a pure FRW metric to describe a bound system, there are some papers that take the approach of using for instance a Schwarzschild De-sitter metric. These approaches can be justified more rigorously if one imagines that the dark matter and dark energy are isotropically distributed, and that the lumpiness is only in the normal matter.

This approach won't model effects due to "lumpiness" in the dark matter, for instance, but one can probably gain some insight into the effects of lumpiness in the dark matter by the effects of lumpiness in the non-dark matter.

The whole dark matter issue is rather annoying if one isinterested in gravity - basically, the source of most of the gravity in the universe appears to be invisible :-(.
 
  • #69
I'm not quite sure what your point is. A hypothetical universe where everything was inititally redshifting, continuously evolving towards less and less redshift, then started to blueshift is imaginable. Furthermore, it is imaginablie in the context of GR - such a universe would have a matter density over the critical, and would be a universe ending in a "big crunch".
Your assumption of a 'big crunch' would be true if you assumed a 'big bang'

I don't understand why you think the experimental data that says that the universe is expanding and that the expansion is accelerating is "frivolous".
I'm not saying that an accelerating expansion is frivolous. Only that if the assumption posted earlier by me were true, that the expansion of space is a frivolous thought. Do you consider the idea of greater masses evolving to even greater masses as frivolous? It is at least a logical progression one might expect irrespective of other known measurements.
My way of creating new angles by which to look at the same thing. In other words - If galaxy clusters are to eventually cluster themselves, what model of a universe would bring this about? Big bang does not fit this bill. This is just thinking out of the box that most of us put ourselves in, and I leave the box because all six sides represent dead ends.

A model that produces an evolving scenerio as described is possible by the way. Doesn't make it right ... but possible?
 
  • #70
Castlegate said:
Do you consider the idea of greater masses evolving to even greater masses as frivolous? It is at least a logical progression one might expect irrespective of other known measurements.
My way of creating new angles by which to look at the same thing. In other words - If galaxy clusters are to eventually cluster themselves, what model of a universe would bring this about? Big bang does not fit this bill. This is just thinking out of the box that most of us put ourselves in, and I leave the box because all six sides represent dead ends.

A model that produces an evolving scenerio as described is possible by the way. Doesn't make it right ... but possible?

Hmm the current model of the universe predicts that mass gets increasingly lumpy as time goes on. Lumps of mass do indeed get more massive as time goes on, clusters form etc etc. I don't follow your previous logic as to how this is a problem but rest assure that far from being incompatible with the Big Bang it is a prediction (and observation!) of current cosmology.
 
  • #71
Castlegate said:
Your assumption of a 'big crunch' would be true if you assumed a 'big bang'
What do you mean by this? Are you meaning to say that if we assume a big bang, then this implies a big crunch in the future? If you are, then this is not true!
 
  • #72
Wallace said:
The point is though that there is not expansion to 'overcome' since the 'expansion' is merely the result of the metric formed by a homogeneous and isotropic mass distribution. If the mass dosn't obey these principles we shouldn't be surprised that we don't see any 'expansion'.

But the expansion is seen on scales where the mass distribution is far from homogeneous and isotropic - namely in the vicinity of or even within the local group of galaxies. Moreover, the Hubble law is obeyed tightly even at this (cosmologically speaking) local scale, and the local Hubble parameter is of the same order as the global one. This problem of "the quiet local Hubble flow" was first identified by Sandage, and it is still an unsolved problem.

For observational results and references to the original papers, see

T. Ekholm et al., Astron. & Astrophys. 368, L17 (2001) (astro-ph/0103090).
 
  • #73
Sure, so there is no harsh cut-off point where the metric goes from FRW suddenly to some other non-expanding form. I would have expected that the expansion would not be dominant on the scale of the local group, so that results is unexpected for me. Thanks for pointing it out, I will have to follow this up.

It remains that case though, that as the local region becomes more and more inhomogenous, the metric must have less and less 'FRWness' in it. The expansion most certainly does not occur on galactic scales or smaller, such as the scale of a solar system for instance.
 
  • #74
Wallace said:
Sure, so there is no harsh cut-off point where the metric goes from FRW suddenly to some other non-expanding form. I would have expected that the expansion would not be dominant on the scale of the local group, so that results is unexpected for me. Thanks for pointing it out, I will have to follow this up.

It remains that case though, that as the local region becomes more and more inhomogenous, the metric must have less and less 'FRWness' in it. The expansion most certainly does not occur on galactic scales or smaller, such as the scale of a solar system for instance.

For sure, it seems that some realistic idea are coming to the fore
.
 
  • #75
Old Smuggler said:
But the expansion is seen on scales where the mass distribution is far from homogeneous and isotropic - namely in the vicinity of or even within the local group of galaxies. Moreover, the Hubble law is obeyed tightly even at this (cosmologically speaking) local scale, and the local Hubble parameter is of the same order as the global one. This problem of "the quiet local Hubble flow" was first identified by Sandage, and it is still an unsolved problem.

For observational results and references to the original papers, see

T. Ekholm et al., Astron. & Astrophys. 368, L17 (2001) (astro-ph/0103090).

I've followed this up, it looks like this was a unfortunately timed paper, coming out just a month or two before the HST key project to measure H0. This paper uses a best guess for H0 of just over 50 km s^{-1} Mpc^{-1} substantially lower than the 72 km s^{-1} Mpc^{-1} found from the Hubble key project. This significantly changes the articles conclusions since it really shows that the local group Hubble diagram will not match the slope of the global expansion rate very well at all. I think this is closer to what I would have expected.
 
  • #76
You may be interested in the references mentioned in this post.
 
  • #77
Wallace said:
I've followed this up, it looks like this was a unfortunately timed paper, coming out just a month or two before the HST key project to measure H0. This paper uses a best guess for H0 of just over 50 km s^{-1} Mpc^{-1} substantially lower than the 72 km s^{-1} Mpc^{-1} found from the Hubble key project. This significantly changes the articles conclusions since it really shows that the local group Hubble diagram will not match the slope of the global expansion rate very well at all. I think this is closer to what I would have expected.

But they didn't measure the Hubble parameter; rather they took a value of 57 km/sMpc as
an input for their model. While it is reasonable to assume that the numbers would change
somewhat if a different input value were chosen, the main results should not be critically
dependent on this. That is, the linearity of the local Hubble law and the small local velocity
dispersion around it should still hold.

As Hellfire pointed out, the mystery of the quiet local Hubble flow could have an explanation in dark energy, suppressing the growth of velocity fluctuations. However, this explanation is not sufficient, since the parameter values necessary to achieve this would
be incompatible with other observational tests. For details, see

M. Axenides and L. Perivolaropoulos, Phys. Rev. D 65 127301 (2002) (astro-ph/0201524).

So what the observations of the velocity field of galaxies in the vicinity of the local group
is telling us, is that there is no obvious link between the expansion and the clumpiness of the Universe. Thus the fact that the Universe is even more inhomogenous on smaller
scales such as galaxies and planetary systems, is in itself not a sufficient argument
to conclude that the expansion cannot exist and be detectable on such scales.
 
  • #78
going back to the analogies...

...has anyone equated space expanding to a cell dividing ?

imagine a single red cell dividing in two. Those 2 red cells then split, but instead split into white cells and every division there after is also white, such that there are only ever 2 red cells. The faster the white cells divide exponentially, pushes the 2 red cells ever further apart and faster...

...it'd make a great cartoon i reckon, cos in the bigger picture you'd see that the 2 red cells are moving apart faster than the rate at which any single white cell is dividing at

now when there weren't many white cells separating the 2 red cells someone living on one red cell shined a torch in the direction of someone on the other red cell, but as the distance between the two cells increased, the light from the torch had to travel further and by a strange coincidence turned red itself...:biggrin:
 
  • #79
This doesn't seem like a very helpful analogy.
 
  • #80
...so its no more or less helpful than the raisin and balloon one. Care to explain why ?

watching cells divide would make for a better cartoon though. Theres just something about how they do that and how space is created which i find intriguing...

...like reconstituting matter from one thing to another in real time
 
  • #81
Hell_SD said:
...less helpful than the raisin and balloon one. Care to explain why ?

watching cells divide would make for a better cartoon though.
I agree with Wallace about cells analogy not helpful---think it is very likely to be harmful to understanding.
with pennies on the balloon, you go thru the exercise of imagining the pennies all drifting apart and then the all-important final step is IMAGINE THE BALLOON ISN'T THERE.

Picture the pennies all receding from each other, their separation distances increasing by some percentage with each time tick

and then imagine the rubber skin isn't there!

============

likewise if you use the raising dough analogy you should, at the end, imagine that the dough is not there

all there is is increasing distances between raisins
=============
the pennies, or the raisins, are the analogs of GALAXIES, where are the galaxies in your analogy?
=============

I would say your "cells" analogy is mind-damaging and pernicious because it tends to mislead people into thinking that space is a "something" like cells. and it gets mentally messy when you imagine finally that all the cells vanish from existence, then what is left?
 
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  • #82
marcus said:
I would say your "cells" analogy is mind-damaging and pernicious because it tends to mislead people into thinking that space is a "something" like cells. and it gets mentally messy when you imagine finally that all the cells vanish from existence, then what is left?

fair enough but surely it's no more messy than the actuality of distances between objects increasing faster than the speed of light without the objects themselves moving...

...and considering there is supposed to be a universal speed limit based on how fast light travels through space which supposedly can't be exceeded or asking the messy question of where does this extra space come from ?

i just like the organicness of cells dividing so could you please tell me why space isn't like cells ? Whats to stop there being a unit of something which appears and vanishes at superluminal speed leaving space as it's residue ?
 
  • #83
Hell_SD said:
fair enough but surely it's no more messy than the actuality of distances between objects increasing faster than the speed of light without the objects themselves moving...

...and considering there is supposed to be a universal speed limit based on how fast light travels through space which supposedly can't be exceeded or asking the messy question of where does this extra space come from ?
...

you sound pretty confused HSD. I don't know what to advise you or where you could begin trying to get straightened out. I can't take time to try but maybe someone else can help you.

you are mixing up SR and GR. the speed limit in SR does not apply globally to rates of distance change in GR. you are mixing up recession speed with relative motion within one local framework

there is NOT supposed to be a universal speed limit that applies to recession speeds. if someone told you that they lied, or were mistaken, or maybe you just misinterpreted. (all that kind of talk is with SR only and SR has a very restricted applicability, if you apply it outside its area of validity it gives nonsense)

there is NO problem of "where extra space comes from" because space is not a material substance-----it is just the distances between things a web of geometric relations----you DONT HAVE TO MAKE MORE.

you mistakenly assert that this is messy, I do not see that anything i am telling you is messy.

between things that are not bound together there is no reason to expect distances to stay the same, in fact large scale distances tend to increase at a certain percentage rate----there is nothing messy or funny about this and no reason to expect it to not be the case---and in fact it is how the world is.

largescale distances typically increase by 1 percent about every 140 million years-----so naturally the longer they are to begin with the faster they increase in absolute terms---that's how percents work.
so naturally some long distances are increasing faster than any given speed, you can always pick a distance long enough that it is increasing faster than c.

Unless you immediately come around and stop talking nonsense i will have to give up on you, and I do not expect you to. So maybe someone else will be willing to try to explain. I hope so.
 
  • #84
distances between objects increasing faster than the speed of light without the objects themselves moving

c'mon marcus that is a hell of a concept to try and wrap your head around...

the fact that the objects aren't moving apart at superluminal speed but that space is growing between them at faster than lightspeed while maintaining that nothing can go faster than c

...sounds messy so surely I have a right to be confused ?
 
  • #85
Well there are theories that say space is nothing. So, it might be that space can move with speeds > c.
 
  • #86
Dividing cells is an absolutely horrible analogy...no offense. It seems to me that the main point of the discussion was to try and describe increasing distances without implying that space itself was driving it apart. Describing space as white cells in this analogy defeats that purpose and implies that space is like matter.

I've been struggling to remember what this gadget is called (perhaps someone can help me out) but if anyone has ever seen these toys that are a lattice type structure with moveable joints that when fully contracted is like a ball. When you pull it apart, it expands in size uniformly to many times it's original size. If you can pictue this and also picture each joint as a galaxy, I've always thought that would be a decent visualization of an expanding universe...:rolleyes:
 
  • #87
Hell_SD said:
distances between objects increasing faster than the speed of light without the objects themselves moving

c'mon marcus that is a hell of a concept to try and wrap your head around...

the fact that the objects aren't moving apart at superluminal speed but that space is growing between them at faster than lightspeed while maintaining that nothing can go faster than c

...sounds messy so surely I have a right to be confused ?

Superluminal recession is something that easily causes confusion. The issue is that velocity is the rate of change of distance and with but in GR neither distance or time are trivial concepts. The distance that we use in FRW cosmology is most commonly the proper distance, and if we look at the rate of change of this with 'cosmic time' (the time as measured by co-moving observers) we note that this velocity exceeds c for sufficient distance from the origin.

All this tells us is how one of many different possible definitions of distance change. If you accept the FRW metric then you have to live with that fact. Other metrics that use difference co-ordinates but make the same physical predictions do not contain any apparent superluminal recession.

You need to realize that your everyday notion of distance doesn't work on cosmological scales, and hence your everyday intuition is useless.
 
  • #88
If we want to measure distances in our own galaxy, we can use a rigid ruler,
and we can get quite an accurate measurement from some point (earth) +,- bodies motion (orbits) within the galaxy.
If we want to measure between galaxies, we have to throw away the rigid ruler and use a flexible one, the rate of flex (stretch) depends on distance from our vantage point, the rate of stretch increases with distance.
The stretch factor is not considered as a (speed) just an increase in the total volume we, the universe exists in.
This sounds total nonsense, but may be i have the above wrong?
 
  • #89
Another paper.

arXiv:0707.1350 (cross-list from gr-qc) [ps, pdf, other]
Title: Cosmological expansion and local physics
Authors: Valerio Faraoni, Audrey Jacques (Bishop's University)
Comments: 17 pages, LaTeX, to appear in Phys. Rev. D
Subjects: General Relativity and Quantum Cosmology (gr-qc); Astrophysics (astro-ph)
The interplay between cosmological expansion and local attraction in a gravitationally bound system is revisited in various regimes. First, weakly gravitating Newtonian systems are considered, followed by various exact solutions describing a relativistic central object embedded in a Friedmann universe. It is shown that the ``all or nothing'' behaviour recently discovered (i.e., weakly coupled systems are comoving while strongly coupled ones resist the cosmic expansion) is limited to the de Sitter background. New exact solutions are presented which describe black holes perfectly comoving with a generic Friedmann universe. The possibility of violating cosmic censorship for a black hole approaching the Big Rip is also discussed.
 
  • #90
The issues arising with measuring the distance to distant galaxies are not really related to the problem of constructing a rigid ruler (though of course a rigid ruler is an idealization - the most rigid ruler that's actually possible would be counting the wavelengths on a lightbeam, which is only approximately rigid. This is essentially a limiting case when the velocity of sound in the ruler is equal to 'c'.)

Rather, the issue with measuring distance it is the problem of "what curve" to measure the length of. The usual notion of distance proceeds as follows - one takes space-time, and separates it out into space and time. One then measures the distance in some hypersurface of constant time.

Unfortunately, the split of space-time into space and time is in general arbitrary and depends on the choice of coordinates.

Note that the usual notion of distance ("proper distance") defined in this manner (measuring the distance along a curve of constant cosmological time) does not actually measure the distance along a straight line (or the equivalent of a straight line in a curved space-time, a space-like geodesic).

This is because a curve of constant cosmological time connecting two points in a FRW universe is not a "straight line", i.e. it is not a geodesic.
 
  • #91
The so called 'physical' distance in cosmology doesn't have the status of invariance (independence of coordinate system) like the line element ds^2 because the 'physical' distance is a coordinate quantity.

It can be measured if you have a gazillion of comoving observers in straight line from you to the point where you want to measure. Those observers have clocks that all show the 'cosmic' time which is a coordinate time in FRW metric. You simply tell them at given fixed cosmic time to record the distance to the closest comoving observer. Assuming that distance is small it will be the line element ds. Then you tell them to report the distances to you and you add them up getting the coordinate distance to the object at that time. Basically this is integration of ds over a specified curve which as pervect pointed out is NOT a geodesic.
 
  • #92
I recommend the following article :

Misconceptions about the Big Bang
Baffled by the expansion of the universe? You're not alone. Even astronomers frequently get it wrong
By Charles H. Lineweaver and Tamara M. Davis

http://www.sciam.com/article.cfm?articleID=0009F0CA-C523-1213-852383414B7F0147


As far as explaining a complex issue in a precise, didactic and relevant manner, I haven't found a better paper so far...
 
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  • #93
"photons are massless but they do have energy"

I am sure this is a stupid question, but if M=E/c^2 and E is nonzero, how can M be zero?

dilletante
 
  • #94
It can't. That equation has nothing to do with photons.
 
  • #95
The full equation for the relativistic energy of a particle is (well not completely general, but more verbose than the famous short version) is:
<br /> E^2=M^2c^4 + p^2c^2<br />
where p is the momentum of the particle

This reduces to E=Mc^2 when the momentum is small (i.e. particle isn't moving or is not moving very fast). Photons do have a momentum, but not rest mass, so for them

<br /> E^2=p^2c^2
<br /> E=pc<br />
 
  • #96
Thank you Wallace, your explanation is concise and clear.
 
  • #97
It could be that "space expands" is an unfortunate popularization choice of words because space is not a substance that can expand.

This sounds very categorical but is there really unanimous agreement with this? We assume space is not a "substance" but yet it contains energy, can create virtual particles, and there seems to be agreement that you can curve it to explain gravity -- why then can you not "stretch" it?

dilletante
 
  • #98
This thread is extremely interesting...but at the end of the day, it proves one thing - that we (layperson AND scientific professional) don't really understand anything!? It all amounts to fumbling with words. What we need is a model we can picture in our heads, something we can visualize. If the universe is beyond human understanding/visualization, why do we bother?

Space is "nothingness" but it is stretching and is infused with "virtual matter" popping in & out of existence...? Huh? The universe came out of "nothingness"? Huh?

Nothing makes sense - or should I say, "nothing" doesn't make sense. I find the universe we are in disturbing - frightening!

We are "made of star dust" and are intimately/subatomically connected to this universe, and yet we seem like aliens/strangers/outsiders to it all...

Plus, there seems to be so much disinformation out there, so much noise clogging up the signal... Stark contradictions, ambiguities, unspoken assumptions... It's hard/impossible to find answers...

From a layman's point of view (me), I am completely unsatisfied with our state of knowledge today.

Damn, I'm in a miserable mood today!
 
  • #99
mattex said:
This thread is extremely interesting...but at the end of the day, it proves one thing - that we (layperson AND scientific professional) don't really understand anything!? It all amounts to fumbling with words. What we need is a model we can picture in our heads, something we can visualize. If the universe is beyond human understanding/visualization, why do we bother?

Space is "nothingness" but it is stretching and is infused with "virtual matter" popping in & out of existence...? Huh? The universe came out of "nothingness"? Huh?From a layman's point of view (me), I am completely unsatisfied with our state of knowledge today.
a good bit of the problem comes from using the English language instead of math.
we all expect "understanding" to correspond to English sentences and dictionary definitions

IndoEuropean root language goes back to what, before 5000 BC probably.
You expect distance between two stationary locations, village A and village B, to stay constant.

in the GR model of dynamic geometry it CANNOT stay constant, unless A and B are bolted onto some material framework. If it is galaxy A and galaxy B , not bound together, it MUST change. It is of the nature of distance to change and the GR main equation describes how.

But this is not part of the 10,000 year old linguistic tradition to which English belongs. So we think it is confusing.

So be of good cheer Mattex. It is just some obsolete language interfering with your contentment.
 
  • #100
No, it's not increasing distance between 2 galaxies that is the problem. It is increasing distances between ALL galaxies! How can this be? Do we really know?

It's damn frustrating! Nothing adds up! Does the universe curve round on itself? Or is it flat & infinite? What is going on? Why aren't people disturbed?
 
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