How Does the Expansion of the Universe look?

In summary, the conversation discusses the confusion and potential inaccuracies in a statement made by theoretical physicist Lawrence Krauss about the expansion of the universe and the possibility of losing sight of objects traveling faster than light. It also touches on the concept of cosmological red shift and the diminishing density of matter in the early universe. The conversation concludes with a suggestion to read a more comprehensive essay by Krauss and a reminder not to take poetic statements too seriously.
  • #1
Berenices
22
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Hey all,
I was reading a webpage which I found rather confusing:
http://www.dailygalaxy.com/my_weblog/2015/06/todays-galaxy-insight-the-lonely-galaxies.html
The problem I found with this is that the guy (who is a famous theoretical physicist) is stating that because the objects will be traveling FTL we will lose sight of them, forever.
However this would only make sense if the universe expanded intuitively, if it did, we should not be able to see the CMB!
To my understanding, because light has such incredibly long travel times on scales as large the visible universe the pictures we look at are not things, say, twelve billion ly away, they're pictures of EM waves that have traveled for twelve billion ly across an expanding universe, because the actual objects are receding away, the light is red-shifted. To add to this, matter actually gets more packed together as you look back in cosmic time.

How then, can the entire universe dissipate away and leave no trace of itself after such a short time in cosmic terms? Am I missing out on something? Did I misinterpret the statement? Or am I right, if this is the case; why would a theoretical physicist tell a bit of a lie just to push an idea that we live in a special time?
 
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  • #2
Berenices said:
However this would only make sense if the universe expanded intuitively, if it did, we should not be able to see the CMB!
First of all, it is not clear what you mean by "expanding intuitively". Second, it is not clear how you think this would infer that the CMB could not be seen. Rest assured that everything is self consistent.

Berenices said:
because the actual objects are receding away, the light is red-shifted
Cosmological red shift is more accurately due to the expansion of space leading to longer wavelengths. Both source and receiver can be at rest in comoving coordinates.
 
  • #3
Berenices said:
Hey all,
I was reading a webpage which I found rather confusing:
http://www.dailygalaxy.com/my_weblog/2015/06/todays-galaxy-insight-the-lonely-galaxies.html
...
...
How then, can the entire universe dissipate away and leave no trace of itself after such a short time in cosmic terms? Am I missing out on something? Did I misinterpret the statement? Or am I right, if this is the case; why would a theoretical physicist tell a bit of a lie just to push an idea that we live in a special time?
Larry Krauss writes popular books and he naturally wants them to sell, and reporters in media can quote him out of context and get things wrong, and stuff gets sensationalized.

Here is an essay that Krauss and a colleague submitted to judges in an annual Gravity Research Essay Contest. It says something like what you were wondering about but with more careful conditions, reservations, qualifications. It is free. We don't have to buy some popular-written book that oversimplifies. We can all look at the same firsthand writing and try to make sense of it.
It is still slightly sensationalist but it is more careful because going to a professional audience:
http://arxiv.org/abs/0704.0221
The Return of a Static Universe and the End of Cosmology
Lawrence M. Krauss (1,2), Robert J. Scherrer (2) ((1) Case Western Reserve University, (2) Vanderbilt University)
(Submitted on 2 Apr 2007 (v1), last revised 27 Jun 2007 (this version, v3))
We demonstrate that as we extrapolate the current ΛCDM universe forward in time, all evidence of the Hubble expansion will disappear, so that observers in our "island universe" will be fundamentally incapable of determining the true nature of the universe, including the existence of the highly dominant vacuum energy, the existence of the CMB, and the primordial origin of light elements. With these pillars of the modern Big Bang gone, this epoch will mark the end of cosmology and the return of a static universe. In this sense, the coordinate system appropriate for future observers will perhaps fittingly resemble the static coordinate system in which the de Sitter universe was first presented.
5th prize 2007 Gravity Research Foundation Essay Competition, to appear, GRG October 2007;
 
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  • #4
Berenices said:
Hey all,
I was reading a webpage which I found rather confusing:
http://www.dailygalaxy.com/my_weblog/2015/06/todays-galaxy-insight-the-lonely-galaxies.html
The problem I found with this is that the guy (who is a famous theoretical physicist) is stating that because the objects will be traveling FTL we will lose sight of them, forever.
The light can never reach us - or it is infinitely red-shifted.

However this would only make sense if the universe expanded intuitively, if it did, we should not be able to see the CMB!
Why not? All it means is that the CMB we see around us comes from closer than the FTL edge.

To my understanding, because light has such incredibly long travel times throughout the visible universe the pictures we look at are not things, say, twelve billion ly away, they're pictures of EM waves that have traveled for twelve billion ly across an expanding universe, because the actual objects are receding away, the light is red-shifted. To add to this, matter actually gets more packed together as you look back in cosmic time.
Not all light has very long travel times - the light from your computer screen takes very little time to reach you.
The red-shift is due to the expansion during the intervening time - not so much the speed of the emitting object. i.e. it is not a doppler effect.
Certainly the current models have a more dense distribution of matter in the earlier Universe.

How then, can the entire universe dissipate away and leave no trace of itself after such a short time in cosmic terms?
If that's a short time then I shudder to think what you'd call a long time!
It did not "dissipate away", it expanded. As space expands, the clumps of matter get further apart and so the mas-density decreases. That's just geometry.

Am I missing out on something? Did I misinterpret the statement?
You seem to have got the statement about FTL OK - it's the nature of the CMB you don't understand properly.
http://www.thenakedscientists.com/forum/index.php?topic=46907.0

The bit about being in a special time is a bit poetic - don't take it too much to heart. Physicists can get a bit carried away.

[edit] the others beat me to it.
 
  • #5
"First of all, it is not clear what you mean by "expanding intuitively". Second, it is not clear how you think this would infer that the CMB could not be seen. Rest assured that everything is self consistent."
Just because of the light travel time having a large effect, I read somewhere that the calculation is that objects are receding ftl beyond 11b ly..
According to this post: https://www.physicsforums.com/threads/why-can-we-still-detect-the-cmb.801895/,
The expansion of the universe should not result in the CMB becoming undetectable.

EDIT: sorry for my mis-clarification, I wasn't saying that CMB radiation comes from beyond the FTL edge, I was saying that it must have been emitted before this time, and that we are not seeing the distance, only the product of the light travel time.
 
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Related to How Does the Expansion of the Universe look?

1. What is the expansion of the universe?

The expansion of the universe refers to the continuous increase in the distances between galaxies and other cosmic structures. This expansion is caused by the force of dark energy, which is thought to make up around 70% of the total energy density of the universe.

2. How does the expansion of the universe look?

The expansion of the universe cannot be physically seen, as it occurs on a cosmic scale that is far beyond our human perception. However, scientists can measure the expansion by observing the redshift of light from distant galaxies, which indicates that they are moving away from us.

3. Is the expansion of the universe uniform?

No, the expansion of the universe is not uniform. While all objects are moving away from each other, the rate of expansion can vary depending on the distance between the objects and the amount of dark energy in their surrounding regions. This is known as the "Hubble flow."

4. Will the expansion of the universe ever stop?

Current scientific evidence suggests that the expansion of the universe will continue indefinitely, as the amount of dark energy in the universe is thought to be increasing over time. This means that the expansion rate may even accelerate in the future.

5. How does the expansion of the universe affect our daily lives?

The expansion of the universe does not have any direct impact on our daily lives, as it occurs on such a large scale. However, understanding the expansion can help us better understand the origins and fate of the universe, and the forces at work in our universe. It also has implications for the study of cosmology and the search for extraterrestrial life.

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