Is Expansion the Same as Contraction?

In summary, the conversation discussed the difference between expanding outwards and contracting inwards and how it relates to the concept of time dilation and length contraction at relativistic speeds. While expansion and contraction can be observed in materials like metals, it is not comparable to the distribution of numbers on the number line. The conversation also touched on the FLRW family of cosmological GR solutions, which allows for both expanding and contracting universes. It was also mentioned that the terms "outwards" and "inwards" are redundant and can be removed from the question. The conversation ended with a mention of T-Duality and the idea that the size of the universe would always appear to be expanding due to the difference from 1 increasing with time.
  • #1
theoretical symmetry
How do you tell the difference of expanding outwards and contracting inwards?

Part of my intuition tells me that it would be impossible to tell the difference.

If you are on the natural numbers heading from zero to infinity I might say that is expanding outwards.

So if you are sitting at zero and moving to negative infinity then that would seem like contracting inwards. However you would leave the positive numbers behind and have negative numbers ahead but since you are moving forward it would seem natural to label those numbers as positive and the others as negative.

So the forward arrow of time would imply that the numbers covered would always appear as the natural numbers.

The larger part of my intuition tells me that I could be way far off and not even know it without checking with PF.

Thoughts?
 
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  • #2
theoretical symmetry said:
How do you tell the difference of expanding outwards and contracting inwards?
Expansion creates red shift (which we observer), contraction would create blue shift (which we do not observe), and that is just one of the ways that we know the universe is expanding.
 
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  • #3
Your question is hard to answer. Expansion and contraction of materials like metals is classically a matter of temperature. But as you posted in the relativity theory forum, I suspect it is about time dilation and length contraction at relativistic speeds. But this cannot be explained by or even compared to the distribution of numbers on the number line, no matter which way you "walk" or "how far".

It is due to different perspectives which depend on the rest frame (coordinate system) you observe an object in motion. Have you tried to understand the Wikipedia entry about it?

In any case, we need a more specified question for an answer. Otherwise it would lead to a lecture about special relativity, which cannot be done here. May I ask you about your background, in order to provide an appropriate link to what can be read about it?
 
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  • #4
I was leaning more towards the notion that a red shift would be observed even in a contacting universe because from within that reference frame everything would appear to be expanding.
 
  • #5
fresh_42 said:
Your question is hard to answer. Expansion and contraction of materials like metals is classically a matter of temperature. But as you posted in the relativity theory forum, I suspect it is about time dilation and length contraction at relativistic speeds. But this cannot be explained by or even compared to the distribution of numbers on the number line, no matter which way you "walk" or "how far".

It is due to different perspectives which depend on the rest frame (coordinate system) you observe an object in motion. Have you tried to understand the Wikipedia entry about it?

In any case, we need a more specified question for an answer. Otherwise it would lead to a lecture about special relativity, which cannot be done here. May I ask you about your background, in order to provide an appropriate link to what can be read about it?
Undergraduate physics / mathematics
 
  • #6
I was thinking of it on a numberline as a bunch of particles moving at various speeds. Everything starts off at zero and tends to infinity Pick a particle and measure other particles since they are all moving in the same direction it will always seem like an expansion even if everything tends to negative infinity.
 
  • #7
theoretical symmetry said:
I was thinking of it on a numberline as a bunch of particles moving at various speeds. Everything starts off at zero and tends to infinity Pick a particle and measure other particles since they are all moving in the same direction it will always seem like an expansion even if everything tends to negative infinity.
This sounds a bit like the light clock, which is explained in the article I linked to. You will have to determine a rest frame, in which you observe the particles, e.g. not moving at ##0## or co-moving with one particle. But what should expand or contract? Particles don't have a size, but their specific time is different from yours. This experiment might be interesting in the context: http://web.mit.edu/8.13/www/JLExperiments/JLExp14.pdf
 
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  • #8
Thanks. I am going to read up on the info provided and will return with any more questions or perhaps a rephrasing of the initial question to better assist you in answering it. I appreciate all the responses and links.
 
  • #9
theoretical symmetry said:
I was leaning more towards the notion that a red shift would be observed even in a contacting universe because from within that reference frame everything would appear to be expanding.
OK, you've got me completely flummoxed with that statement. I can't imagine how you arrive at that conclusion since it seems to me to be self-contradictory. What am I missing?
 
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  • #10
theoretical symmetry said:
I was leaning more towards the notion that a red shift would be observed even in a contacting universe
No, that is essentially the definition of an expanding universe.
 
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  • #11
theoretical symmetry said:
I was leaning more towards the notion that a red shift would be observed even in a contacting universe because from within that reference frame everything would appear to be expanding.
No, this is just wrong. FLRW family of cosmological GR solutions allows for contracting universes as well as expanding. The former have blue shift increasing with distance for comoving sources, while latter have redshift.
 
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  • #12
theoretical symmetry said:
How do you tell the difference of expanding outwards and contracting inwards?

Take out the words "outwards" and "inwards"; they are redundant. Then ask the question again; is the answer now obvious?
 
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  • #13
phinds said:
OK, you've got me completely flummoxed with that statement. I can't imagine how you arrive at that conclusion since it seems to me to be self-contradictory. What am I missing?
T-Duality? I figured (wrongly) that if this were true then we wouldn't know if our universe has a very large radius or a very small one. So universe expanding for 46 light years to it's current radius R should be the same size as if it was contracting to 1/R. I thought would always appear expanding because the difference from 1 increases with time.
 
  • #14
theoretical symmetry said:
T-Duality? I figured (wrongly) that if this were true then we wouldn't know if our universe has a very large radius or a very small one. So universe expanding for 46 light years to it's current radius R should be the same size as if it was contracting to 1/R. I thought would always appear expanding because the difference from 1 increases with time.
I have no idea what any of what you just said means.
 
  • #15
phinds said:
I have no idea what any of what you just said means.
From wikipedia "In theoretical physics, T-duality is an equivalence of two physical theories, which may be either quantum field theories or string theories. In the simplest example of this relationship, one of the theories describes strings propagating in an imaginary spacetime shaped like a circle of some radius R, while the other theory describes strings propagating on a spacetime shaped like a circle of radius proportional to 1/R}. The two theories are equivalent in the sense that all observable quantities in one description are identified with quantities in the dual description."
 
  • #16
theoretical symmetry said:
From wikipedia "In theoretical physics, T-duality is an equivalence of two physical theories, which may be either quantum field theories or string theories. In the simplest example of this relationship, one of the theories describes strings propagating in an imaginary spacetime shaped like a circle of some radius R, while the other theory describes strings propagating on a spacetime shaped like a circle of radius proportional to 1/R}. The two theories are equivalent in the sense that all observable quantities in one description are identified with quantities in the dual description."
Ah. Well that explains "T-duality". Thanks. I still have no idea what that has to do with the universe expanding and not contracting.
 
  • #17
theoretical symmetry said:
If you are on the natural numbers heading from zero to infinity I might say that is expanding outwards.

So if you are sitting at zero and moving to negative infinity then that would seem like contracting inwards. However you would leave the positive numbers behind and have negative numbers ahead but since you are moving forward it would seem natural to label those numbers as positive and the others as negative.
theoretical symmetry said:
I was thinking of it on a numberline as a bunch of particles moving at various speeds. Everything starts off at zero and tends to infinity Pick a particle and measure other particles since they are all moving in the same direction it will always seem like an expansion even if everything tends to negative infinity.
What you describe as contraction in your example with the number line isn't contraction - it's expansion. Expansion is when the distance between every two arbitrarily chosen points increases with time - it is not when their coordinates become more negative.
If you have a coordinate system in 1-dimensional space (line), where you're at the origin, and you look at some particle sitting to the left (in the negatives), and then look at it later, you get expansion when the distance will have increased. You get contraction when the distance will have decreased.
 
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  • #18
theoretical symmetry said:
So universe expanding for 46 light years to it's current radius R should be the same size as if it was contracting to 1/R.

You cannot have a radius of ##\frac{1}{R}##. It doesn't make sense to speak of such a thing in any context.

Now, it does make sense to speak of a contracting universe, but as has been pointed out several times in this thread, all observations indicate that the universe is expanding, not contracting. In you original post you asked it it were possible to tell the difference and we've told that it is possible, and that it has been done.

Adding the adjectives inward and outward do one of two things: add a redundancy or produce nonsense. Here are the four relevant examples.

An outward expansion (outward is redundant and therefore can be removed without altering the meaning of the phrase).
An inward expansion (nonsense because the inward direction is opposite to the direction of expansion).
An inward contraction (inward is redundant and therefore can be removed without altering the meaning of the phrase).
An outward contraction (nonsense because the outward direction is opposite to the direction of contraction).
 
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  • #19
theoretical symmetry said:
How do you tell the difference of expanding outwards and contracting inwards?

Part of my intuition tells me that it would be impossible to tell the difference.
I feel like you've tied yourself in some sort of logical knot and can't get out or fell down a speculative rabbit hole and can't see how you got here. Please, take a step back, find a balloon, blow it up. That's expansion. Let it go. That's contraction. There is no possible way you could mistake one for the other.
theoretical symmetry said:
So universe expanding for 46 light years to it's current radius R should be the same size as if it was contracting to 1/R. I thought would always appear expanding because the difference from 1 increases with time.
You've [almost] constructed an equation: R=1/R. Now use it! Quite clearly, it can only be valid for R=1. For increasing (expanding) numbers, you have:
2=1/2=False!
3=1/3=False!
4=1/4=False!
Etc.

Clearly, expansion and contraction are not equivalent.
If you are on the natural numbers heading from zero to infinity I might say that is expanding outwards.

So if you are sitting at zero and moving to negative infinity then that would seem like contracting inwards.
Well, there are two easy ways to test this:
1. Plug some negative numbers into your equation and let me know if it produces a valid result.
2. Draw, with your mind, a set of X,Y,Z axes through the center of your balloon and then blow up the balloon. What happens on the negative side of the axes?
 
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Related to Is Expansion the Same as Contraction?

What is expansion and contraction?

Expansion and contraction refer to the increase or decrease in size or volume of a material in response to changes in temperature or pressure.

What causes expansion and contraction?

Expansion and contraction occur due to the movement of molecules within a material. When heated, molecules move faster and take up more space, causing expansion. When cooled, molecules slow down and take up less space, resulting in contraction.

What are some examples of materials that expand and contract?

Most materials, including solids, liquids, and gases, expand and contract with changes in temperature and pressure. Some examples include metals, water, air, and rubber.

How does expansion and contraction affect structures and objects?

Expansion and contraction can cause changes in the size and shape of structures and objects. This can lead to issues such as warping, cracking, and structural damage if not accounted for in the design and construction process.

How is expansion and contraction measured and accounted for?

Expansion and contraction can be measured using instruments such as thermometers and expansion joints. Engineers and designers can also account for these changes by using materials with known expansion and contraction rates, as well as incorporating flexible components and space for expansion in their designs.

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