Understanding the Flat Geometry and Curvature of the Universe

In summary: However, it can wrap around in all directions.The function preserves the Euclidean metric so it is flat.One can think of it as a cylinder made in both directions.
  • #1
Alltimegreat1
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I'm having trouble understanding the terms "flat geometry of the universe" and "baseline curvature of the universe." How can a 3D universe be flat?
 
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  • #2
It is flat in the sense that it has no curvature.

2D geometry can be curved as well. For example, if you draw a triangle on the surface of a sphere (a 2D surface), its interior angles will add up to a number larger than 180 degrees. This is a consequence of the curvature of the space.

Flat space is called Euclidean space, where the interior angles of a triangle add up to 180 degrees, and parallel lines never intersect.

3D space can be flat (i.e., Euclidean) in the sense that parallel lines never meet and keep the same distance from each other.
3D space, doesn't have to be flat though.
If we apply the rules on non-euclidean spaces to 3D, you can get things like parallel lines at one point eventually bending toward each other and intersecting.

The geometry of the Universe usually refers to space and time as a peculiar kind of 4-dimensional system called "space-time". Where spacetime is flat, we see that it obeys the rules of euclidean geometry and spatial relativity. However, the theory of General Relativity says that mass/energy curves or warps spacetime. That means near a massive body, the laws of space and time are non-euclidean.
 
  • #3
jfizzix said:
3D space can be flat (i.e., Euclidean) in the sense that parallel lines never meet and keep the same distance from each other.
Flat is not the same thing as Euclidean.
 
  • #4
Orodruin said:
Flat is not the same thing as Euclidean.
For nearly all intents and purposes, it is.

It's possible for a flat space to wrap back on itself, but this definitely doesn't occur for our observable universe. So as far as we can tell, our universe is very close to Euclidean on large scales.
 
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  • #5
Chalnoth said:
For nearly all intents and purposes, it is.
Definitely not. For the application to cosmology, yes, but flattness and being a Euclidean space are different mathematical concepts.
 
  • #6
Orodruin said:
Definitely not. For the application to cosmology, yes, but flattness and being a Euclidean space are different mathematical concepts.
Perhaps, but that distinction is quite subtle.

Euclidean space and flat space have all of the same measurable properties, except for the possibility that a flat space can potentially wrap back on itself.
 
  • #7
Chalnoth said:
Perhaps, but that distinction is quite subtle.

Euclidean space and flat space have all of the same measurable properties, except for the possibility that a flat space can potentially wrap back on itself.
This is not true either. Flatness is a local concept although it is perfectly possible to have completely flat spaces which do not wrap back on themselves and are not Euclidean. In particular, spaces with non-zero torsion come to mind.

As long as you work in a Riemannian setting with the Levi-Civita connection you might have a point, but the original statement was a blanket statement without any qualifiers and as such is incorrect.
 
  • #8
how can a flat space wrap back on itself?
 
  • #9
Alberto87 said:
how can a flat space wrap back on itself?

A cylinder is the most usual example of such a space. It is flat, but has a cyclic direction.

Note that we are talking about intrinsic curvature here, which is a property of the space itself, not of its embedding into a higher-dimensional space. Extrinsic curvature is something different.
 
  • #10
Orodruin said:
A cylinder is the most usual example of such a space. It is flat, but has a cyclic direction.

Note that we are talking about intrinsic curvature here, which is a property of the space itself, not of its embedding into a higher-dimensional space. Extrinsic curvature is something different.
Ah ok, but it only wraps back in one direction, the second direction cannot, am I right?
It´s not possible for a flat space to be finite and unlimited, isn´t it?
Is the torus a flat space time?
 
  • #11
Alberto87 said:
Ah ok, but it only wraps back in one direction, the second direction cannot, am I right?
It´s not possible for a flat space to be finite and unlimited, isn´t it?
Is the torus a flat space time?
It can wrap around in all directions. A torus is an example - whether it is flat or not depends on the metric you put on it.
 
  • #12
Alberto87 said:
Ah ok, but it only wraps back in one direction, the second direction cannot, am I right?
It´s not possible for a flat space to be finite and unlimited, isn´t it?
Is the torus a flat space time?

The function ##(x,y) \rightarrow 2^{-1/2}(cos(x), sin(x),cos(y),sin(y))## maps the Euclidean plane into a flat torus in ##R^4##. The square [0.2π] x [0,2π] in the plane is bent around in both directions and its opposite edges are identified. A square with opposite edges identified is a torus. The function also preserves the Euclidean metric on the plane so the torus is flat. One can think of it as a cylinder made in both directions.

You are right that you can not wrap the cylinder into a flat torus in 3 dimensions. In 3d one would have to stretch the cylinder and this would create curvature. In 4 dimensions one does not need to do any stretching.
 
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Related to Understanding the Flat Geometry and Curvature of the Universe

What is the geometry of the universe?

The geometry of the universe refers to the overall shape and structure of the universe. It is a fundamental concept in cosmology and is used to describe the curvature of space.

What are the three possible geometries of the universe?

The three possible geometries of the universe are flat, open, and closed. In a flat universe, the overall curvature of space is zero. In an open universe, space has a negative curvature and expands forever. In a closed universe, space has a positive curvature and eventually collapses back on itself.

How do scientists determine the geometry of the universe?

Scientists determine the geometry of the universe through various observations and measurements, such as the cosmic microwave background radiation, the distribution of galaxies, and the rate of expansion of the universe. These data can be used to calculate the overall curvature of space.

What is the significance of the geometry of the universe?

The geometry of the universe has important implications for the fate and behavior of the universe. It can help us understand the overall structure and evolution of the universe, as well as the nature of dark energy and dark matter. It also plays a crucial role in theories of the origin of the universe, such as the Big Bang theory.

Is the geometry of the universe constant?

No, the geometry of the universe is not constant. It can change over time due to the influence of dark energy and the expansion of the universe. In fact, the geometry of the universe has likely changed significantly since the Big Bang and may continue to change in the future.

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