What does it mean when cosmologists say the universe is flat?

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In summary, cosmologists use the term "flat" to refer to the geometry and topology of the universe, meaning that space itself is flat and infinite and that parallel lines will never cross. This is different from the spherical shape of the universe, which refers to the idea that some parts of the universe may be disconnected from others. Additionally, the term "flat" can also refer to the prediction of the theoretical inflation theory, where the energy density of the universe is dominated by something similar to vacuum energy and drives the universe towards a flat state. It is important to note that the shape of the universe is still a topic of debate and research in the scientific community.
  • #1
mannygonzales1
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Hi, I was just wondering if someone could explain to me in detail what cosmologists mean when they say "the universe is flat."

To my understanding it is the geometry and topology of the universe they are referring too. But is space itself a sphere? And everything inside space is geometrically flat and infinite?

Thank you for explaining.
 
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  • #2
Excellent question. I hate the fact they call the Universe flat, spherical or hyperbolic. What they mean is that the Universe would be flat if it had two dimensions. If you fire two beams of light and they travel parallel to each other, they will remain that way forever. If the Universe was open, they would eventually diverge. Someone else will explain this better because I can't get my head around this.

cb
 
  • #3
mannygonzales1 said:
Hi, I was just wondering if someone could explain to me in detail what cosmologists mean when they say "the universe is flat."

To my understanding it is the geometry and topology of the universe they are referring too. But is space itself a sphere? And everything inside space is geometrically flat and infinite?

Thank you for explaining.
It's "flat" in that if you take a constant-time slicing of the universe, that slice is composed of flat space. That is, if you build triangles by holding three points of a loop of string so that the three edges are taut, the angles of that triangle will always add up to 180 degrees, no matter how large the triangle.

By contrast, if you do the same thing across the surface of the Earth (holding the string flat across the surface and pulling it tight), you won't get 180 degrees. For a triangle that stretches from the equator to the north pole and back to the equator 90 degrees from the starting point, the sum of the angles is 270 degrees.
 
  • #4
mannygonzales1 said:
Hi, I was just wondering if someone could explain to me in detail what cosmologists mean when they say "the universe is flat."

To my understanding it is the geometry and topology of the universe they are referring too. But is space itself a sphere? And everything inside space is geometrically flat and infinite?

Thank you for explaining.

..EDIT: 2 different ways in describing flat. (1) Mentioned by Chalnoth, where the geometry of the universe in a parallel lines will never cross, the angles in a triangle will always add up to 180 degress, and the corners of cubes will always make right angles(Euclidean geometry). When they try to measure the baryon acoustic oscillations — waves of particles and energy(baryon wave as ruler). It came to almost flat or 'consistent' to flat(conservative type^^). (2)... The other 'flat' came from the prediction of the theoretical inflation theory - energy density of the universe was dominated by something with an equation of state approximating that of vacuum energy, p < - (1/3)p that eventually drives the universe toward a flat (Omega = 1). There is a growing interest in Inflation side (due to latest result; B-mode polarization) but will see.
 
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  • #5
julcab12 said:
..They have 2 different meaning when referring to flat. (1) mentioned by Chalnoth, where the geometry of the universe in a parallel lines will never cross, the angles in a triangle will always add up to 180 degress, and the corners of cubes will always make right angles(Euclidean geometry). When they try to measure the baryon acoustic oscillations — waves of particles and energy(baryon wave as ruler). It came to almost flat or 'consistent' to flat(conservative type^^). (2)... The other 'flat' came from the prediction of the theoretical inflation theory - energy density of the universe was dominated by something with an equation of state approximating that of vacuum energy, p < - (1/3)p that eventually drives the universe toward a flat (Omega = 1). There is a growing interest in Inflation side (due to latest result; B-mode polarization) but will see.
Those aren't different meanings. They're just different ways to describe it.
 
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Chalnoth said:
Those aren't different meanings. They're just different ways to describe it.

Yes. My bad. Done editing. Thanks for the correction. ^^
 
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So I'd like to ask a question that generally gets me confused, so if one could clarify it for me that would be great.

The universe is flat, in the sense of geometry and topology, so when physicists refer to there being more universes, they refer to them as being bubbles as well as ours. Is space spherical? Is the universe spherical? Or is everything flat?
 
  • #8
mannygonzales1 said:
So I'd like to ask a question that generally gets me confused, so if one could clarify it for me that would be great.

The universe is flat, in the sense of geometry and topology, so when physicists refer to there being more universes, they refer to them as being bubbles as well as ours. Is space spherical? Is the universe spherical? Or is everything flat?
When people are talking about "bubbles" they're not talking about geometry. They're talking about the idea that some parts of the universe are disconnected in some sense from other parts.
 
  • #9
"Bubble universes" are totally unproven, so I'm not sure that everyone who talks about them means the same thing. I personally don't believe in them, but that is an opinion with no facts to back it up, just based on the LACK of facts on the other side of what seems to me to be an unnecessarily complex picture.

Space is NOT spherical. The "bubble" is more like the term "quarter", as used when specifying a region of Paris. It doesn't mean 1/4th the way we normally think of "quarter" meaning, it just means "area". Likewise, "bubble" mean something more like "region".
 
  • #10
So the ACTUAL shape of the universe is flat? Don't mean to bombard with questions.
 
  • #11
To add (to the your knowledge, I hope, not to your confusion) there's another thing about this "flat" business. This is not anything different than what has already been said, it's just a different way of looking at it.

As you may be aware, mass "warps" or "bends" spacetime. This is how the theory of General Relativity was proven, by looking at what seemed like "curved" beams of light from distance stars as it passed our sun during a solar eclipse. There is a famous saying that is a good way to think about the "warping":
mass tells spacetime how to bend and spacetime tells mass how to move

So, it is established that mass bends spacetime. But how about if you get out in a region of space that is as far as possible from all mass (and that can be QUITE far)? Is there anything else that "bends" spacetime? Well not so much that there is something that bends it but rather that a "bend" is part of its characteristics. By "bend", I mean in reference to a Euclidean line. Light around a large mass does not follow a Euclidean line, it "bends" relative to one.

Space ITSELF can have a topology that has a built-in "bend" in this sense. If it does not have such a bend, it is said to be flat. As has been pointed out, if it causes two Euclidean lines to diverge, then it is said to be "open" and if causes them to meet, it is said to be "closed".

It is not known that our universe is flat, but it has been measured as being flat to within something like 3% (I may be a bit off on that and it's probably known to be closer than that now).
 
  • #12
mannygonzales1 said:
So the ACTUAL shape of the universe is flat? Don't mean to bombard with questions.
The question, worded that way, isn't quite specific enough. There are two different aspects of shape:
1. The local curvature.
2. The overall connectedness.

The first is what we mean when we say, "space is flat." The second goes under the name of "topology" and may take some explaining.

In topology, a cube with rounded corners and a sphere are the same thing: you can transform one into the other by stretching and bending without any kinking or tearing.

But a donut is entirely different: you can't transform a donut into a sphere without tearing.

As of right now, what we know is that the observable universe is extremely close to flat in terms of the local curvature. This could mean that our observable universe is just a tiny slice of a gigantic spherical topology, large enough that we can't measure the spherical curvature. It could mean that the observable universe is part of a torus (which doesn't have any overall curvature). Or it might be some other topology altogether. Right now, we just don't know what the overall topology of our universe is, because the observable piece is only a small part of it.
 
  • #13
Chalnoth said:
The question, worded that way, isn't quite specific enough. There are two different aspects of shape:

1. The local curvature.

2. The overall connectedness.
The first is what we mean when we say, "space is flat." The second goes under the name of "topology" and may take some explaining.
In topology, a cube with rounded corners and a sphere are the same thing: you can transform one into the other by stretching and bending without any kinking or tearing.
But a donut is entirely different: you can't transform a donut into a sphere without tearing.
As of right now, what we know is that the observable universe is extremely close to flat in terms of the local curvature. This could mean that our observable universe is just a tiny slice of a gigantic spherical topology, large enough that we can't measure the spherical curvature. It could mean that the observable universe is part of a torus (which doesn't have any overall curvature). Or it might be some other topology altogether. Right now, we just don't know what the overall topology of our universe is, because the observable piece is only a small part of it.

Thank you. Using what you said, is it correct to come to the conclusion that the topology of the universe isn't quite known but the geometry has been found to be flat or a Euclidean Geometry?
 
  • #14
phinds said:
It is not known that our universe is flat, but it has been measured as being flat to within something like 3% (I may be a bit off on that and it's probably known to be closer than that now).

WMAP says:

"We now know (as of 2013) that the universe is flat with only a 0.4% margin of error."

What they mean when they say 'flat to within X percent' is that the total observed density (baryons + dark matter + dark energy) equals the critical density to within X percent.
 
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  • #15
Bill_K said:
WMAP says:

"We now know (as of 2013) that the universe is flat with only a 0.4% margin of error."

What they mean when they say 'flat to within X percent' is that the total observed density (baryons + dark matter + dark energy) equals the critical density to within X percent.
...which is another way to say that the total energy density equals the square of the expansion rate to within that level of accuracy (with a constant conversion factor of ##8\pi G/3##).
 
  • #16
mannygonzales1 said:
Hi, I was just wondering if someone could explain to me in detail what cosmologists mean when they say "the universe is flat."

To my understanding it is the geometry and topology of the universe they are referring too. But is space itself a sphere? And everything inside space is geometrically flat and infinite?

Thank you for explaining.

Let me throw my 2 cents in. Sometimes a certain explanation will just ring true for different people. When i think about the flatness of the universe i try not to think of it as existing either as a sphere or a small cube in an otherwise gargantuan sphere, which may actually be what we live in. I think of Einsteins curvature of space-time due to gravity. Since mass warps space-time into various "shapes" this causes space to curve in on itself. For example the milky way rests in a very large curved region which is not flat and two parallel lines beginning at one end will no longer be parallel at the other due to the warping that all the matter and energy causes as they traverse the galaxy. So think of the milky way as a gigantic, very curved space-time region. It is VERY hard for anything to escape its gravity well due to its curvature. Well just as a region of space, like the milky way can be curved so can the entire observable universe when observed as a whole. However when we look at the entire observable universe there appears to be no overall curvature. The density of matter and energy is too small to create an overall curvature. It looks flat. So in theory two parallel lines will not converge, however in reality they will bend and converge/diverge as they travel through both gravity wells and voids. This is why we observe gravitational lensing. The light from behind massive clusters is bent and converges towards our telescopes. Those lines are not parallel. But on the largest of views space-time shows virtually no curvature and parallel lines never converge or diverge. This is how i think when i think of space-time being "flat". It doesn't necessarily mean we live in a gigantic sphere. I think that question has more to do with whether the universe is finite or infinite which is a different but related question. I think. Any thoughts from anyone? Thanks
 

FAQ: What does it mean when cosmologists say the universe is flat?

What does it mean for the universe to be "flat"?

The term "flatness of the universe" refers to the overall geometry of the universe. In this context, "flat" means that the universe has no overall curvature, similar to a flat sheet of paper. This is in contrast to a "closed" universe, which would have a positive curvature like a sphere, or an "open" universe, which would have a negative curvature like a saddle.

How do we measure the flatness of the universe?

The flatness of the universe can be measured through observations of the cosmic microwave background (CMB), the leftover radiation from the Big Bang. By analyzing the patterns and fluctuations in the CMB, scientists can determine the overall curvature of the universe and thus its flatness.

What are the implications of a flat universe?

A flat universe has significant implications for the fate of the universe. It suggests that the expansion of the universe will continue indefinitely, but at a decreasing rate. This means that the universe will not collapse in on itself, but will continue to expand and cool.

Is there evidence for a flat universe?

Yes, there is strong evidence supporting a flat universe. The most significant evidence comes from the observations of the CMB, which has been found to have a nearly uniform temperature in all directions, indicating a flat geometry. Other evidence comes from studies of the large-scale structure of the universe and the behavior of distant supernovae.

Could the universe have a different geometry in different regions?

Currently, there is no evidence to suggest that the geometry of the universe varies in different regions. The universe appears to be homogeneous and isotropic on a large scale, meaning that it looks the same in all directions and at all locations. However, there may be some small variations in the curvature of the universe, which could be explored further through future observations and research.

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