Understanding a "Flat Universe"

In summary, the concept of a flat universe is often misunderstood as being two-dimensional, when in reality it refers to the principles of Euclidean geometry being applicable. This means that parallel lines never converge and the angles of a triangle add up to 180 degrees. This understanding is crucial in comprehending the current model of the big bang and the evolution of our understanding of the universe. However, this terminology can cause confusion for those without a strong mathematical background.
  • #1
Serpens
5
0
Now I don't quite understand what a flat universe means. Clearly we are not talking about dimensions right? Obviously universe has more than 2 dimensions. So what does flat stand for ? Don't start with Euclidian Geometry please.
 
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  • #2
I'm not sure what you mean by "don't start with Euclidean Geometry" because a flat Universe is completely defined by the aspects of Euclidean Geometry, essentially it follows Euclid's postulates: http://mathworld.wolfram.com/EuclidsPostulates.html. By studying WMAP's representation of the CMB (http://en.wikipedia.org/wiki/WMAP/http://en.wikipedia.org/wiki/Cosmic_microwave_background_radiation ) Cosmologists have concluded with a 2% margin of error that the Universe is spatially flat hence the constant curvature (http://en.wikipedia.org/wiki/Constant_curvature) is [tex]\Omega[/tex]0 = 0. Other forms of geometry for the Universe include Hyperbolic Geometry (http://en.wikipedia.org/wiki/Hyperbolic_geometry) and Spherical/Elliptical Geometry (http://en.wikipedia.org/wiki/Spherical_geometry). The Constant of curvature in these geometries are:
Hyperbolic = [tex]\Omega[/tex]0 = -1
Spherical/Elliptical = [tex]\Omega[/tex]0 = 1
 
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  • #3
As far as I understand it, it is like this: Imagine a strictly fictional 4D Euclidean space (nothing to do with space-time). Now, let us consider hyper-surfaces (i.e. 3D surfaces in 4D space given by some relation [itex]f(x_{1}, x_{2}, x_{3}, x_{4}) = 0[/itex]) that are rotationally invariant, i.e. the functional dependence above is of the form:

[tex]
F(r, x_{4}) = 0, \; r = \sqrt{x^{2}_{1} + x^{2}_{2} + x^{2}_{3}}
[/tex]

Here, we may use an analogy with 3D space and 2D (hyper)surfaces. If they are rotationally invariant around [itex]x_{3}[/itex], then they are of the form [itex]F(\rho, x_{3}) = 0, \; \rho = \sqrt{x^{2}_{1} + x^{2}_{2}}[/itex].

One hypersurface is spherical if:

[tex]
r^{2} + x^{2}_{4} = a^{2}
[/tex]

in analogy to a 3D sphere [itex]\rho^{2} + x^{2}_{3} = a^{2}[/itex].

Another surface is hyperbolic (and open along the [itex]x_{4}[/itex] direction) if:

[tex]
x^{2}_{4} - r^{2} = a^{2}
[/tex]

in analogy to the 3D hyperboloid [itex]x^{2}_{3} - \rho^{2} = a^{2}[/itex].

Finally, a flat hyper-surface perpendicular to the [itex]x_{4}[/itex] direction may be written as:

[tex]
x_{4} = a \Rightarrow x^{2}_{4} = a^{2}
[/tex]

in analogy to a 3D plane perpendicular to the [itex]x_{3}[/itex] direction [itex]x_{3} = a[/itex].

A clever observation is that all of these cases correspond to an implicit functional relationship of the form:

[tex]
x^{2}_{4} + \Omega \, r^{2} = a^{2}
[/tex]

and the different cases correspond to the values:

[itex]\Omega = 1[/itex] - spherical

[itex]\Omega = 0[/itex] - flat

[itex]\Omega = -1[/itex] - hyperbolic

Now, let us return to the question of the metric along this surface. The squared distance between to infinitesimally distant points is still given by the famous Euclidean form:

[tex]
ds^{2} = dx^{2}_{1} + dx^{2}_{2} + dx^{2}_{3} + dx^{2}_{4}
[/tex]

but, not all 4 coordinates are independent because of the above functional relationship (we are fixed on the 3D hyper surface and cannot wander off of it). We can use that relationship to eliminate one of the coordinates, namely [itex]x_{4}[/itex]. Let us differentiate the above relation:

[tex]
2 \, x_{4} \, dx_{4} + \Omega \, 2 \, r \, dr = 0 \Rightarrow dx_{4} = -\frac{\Omega \, r \, dr}{x_{4}}
[/tex]

Furthermore, we can still use spherical coordinates for the remaining three Cartesian coordinates and write:

[tex]
dx^{2}_{1} + dx^{2}_{2} + dx^{2}_{3} = dr^{2} + r^{2} \, \left( d\theta^{2} + \sin^{2}{\theta} \, d\phi^{2} \right)
[/tex]

everywhere. The squared differential of the fourth Cartesian coordinate is:

[tex]
dx^{2}_{4} = \left( -\frac{\Omega \, r \, dr}{x_{4}} \right) = \frac{\Omega^{2} \, r^{2} \, dr^{2}}{x^{2}_{4}} = \frac{\Omega^{2} \, r^{2} \, dr^{2}}{a^{2} - \Omega \, r^{2}}
[/tex]

where we have used the functional relation once more to eliminate the remaining [itex]x^{2}_{4}[/itex]. Combining everything together and simplifying the coefficient in front of [itex]dr^{2}[/itex], we get:

[tex]
ds^{2} = \frac{a^{2} + \Omega \, (\Omega - 1) \, r^{2}}{a^{2} - \Omega \, r^{2}} \, dr^{2} + r^{2} \, \left( d\theta^{2} + \sin^{2}{\theta} \, d\phi^{2} \right)
[/tex]

This metric corresponds to specific classes of non-Euclidean 3D spaces.
 
  • #4
i think serpens asks a good question. it marks a chasm in the understanding of the layscientist (like myself) from the understanding of those with a heavy and appropriate mathematical background.

i bet he's littlerally trying to picture "flat" space in 3d terms and going "what the hell."

i wish that elementary schools and high schools would do a better job of teaching how our model of the big bang has evolved in the last 10 years...
 
  • #5
eliaschristea said:
i think serpens asks a good question. it marks a chasm in the understanding of the layscientist (like myself) from the understanding of those with a heavy and appropriate mathematical background.

i bet he's littlerally trying to picture "flat" space in 3d terms and going "what the hell."

i wish that elementary schools and high schools would do a better job of teaching how our model of the big bang has evolved in the last 10 years...

Calling it a "flat" universe is JARGON. When scientists say "flat", they mean that the principles of Euclidean geometry are applicable (parallel lines never converge, three angles of a triangle add up to 180 degrees etc.). Again for emphasis: Euclidean is what flat means in this context. It does not mean two-dimensional. The OP seems to be wracking his/her brain over a contradiction that just stems from terminology/nomenclature.
 
  • #6
are you a science teacher or something? i wish that when i was in secondary school that notions of time and space, etc, were defined and taught with more of their relativistic signifigance...

a lot gets lost - again for the layperson - in JARGON conflict!
 

What is a "Flat Universe" and how is it different from other types of universes?

A "Flat Universe" refers to a theoretical model of the universe in which the overall geometry is flat, meaning that the angles of a triangle add up to 180 degrees and parallel lines never meet. This is in contrast to a "closed" universe, in which the angles of a triangle add up to more than 180 degrees and parallel lines eventually converge, or an "open" universe, in which the angles of a triangle add up to less than 180 degrees and parallel lines continue to diverge.

How do scientists determine if the universe is flat?

Scientists use various methods to measure the overall curvature of the universe, such as studying the cosmic microwave background radiation, analyzing the distribution of galaxies, and observing the bending of light from distant objects. These methods have provided strong evidence that the universe is indeed flat.

What implications does a flat universe have on the expansion of the universe?

A flat universe suggests that the expansion of the universe is driven by dark energy, a mysterious force that counteracts gravity and causes the universe to expand at an accelerating rate. This is in line with current observations and theories about the expansion of the universe.

Does a flat universe have an edge or boundary?

No, a flat universe does not have an edge or boundary. This is because in a flat universe, space and time are infinite and continuous, meaning there is no physical boundary or edge that marks the end of the universe.

Are there any other theories or models that contradict the concept of a flat universe?

There are some alternative theories and models that propose a non-flat universe, such as the "cyclic model" which suggests that the universe goes through cycles of expansion and contraction, and the "multiverse theory" which suggests that there may be multiple universes with different curvature. However, the flat universe model is currently the most widely accepted and supported by evidence.

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