Is the Universe Flat or Curved?

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Discussion Overview

The discussion centers around the shape of the universe, specifically whether it is flat or curved. Participants explore various models and interpretations of the universe's geometry, addressing theoretical, mathematical, and observational aspects of cosmology.

Discussion Character

  • Debate/contested
  • Exploratory
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants note that observations are consistent with a spatially flat universe, but the extent of its flatness beyond observable limits remains uncertain.
  • One participant references measurements from the COBE and WMAP satellites, suggesting that the universe is either flat or very close to flat, with implications for its curvature over time.
  • Another viewpoint suggests that the concepts of flatness and roundness may be misunderstood, proposing that a universe can be spherical yet flat, depending on its density.
  • A participant introduces a model suggesting a trumpet-like shape for the universe, which is met with skepticism and clarification that this may not accurately represent spatial geometry.
  • There is a discussion about the distinction between local flatness and global geometry, with some arguing that a sphere cannot be globally flat, while others suggest that large spheres may appear locally flat.
  • Some participants challenge the analogy of the universe's shape to that of water, arguing that the question of curvature is valid and significant in understanding the universe's geometry.
  • Concerns are raised about the relevance of discussing the universe's shape in terms of "containers," emphasizing the importance of understanding the curvature on a large scale.

Areas of Agreement / Disagreement

Participants express a range of views on the universe's shape, with no consensus reached. Some agree on the observational evidence for flatness, while others propose alternative models or challenge the interpretations of curvature.

Contextual Notes

Participants highlight the complexity of defining the universe's shape, noting that terms like "flat" and "round" can have different meanings depending on context. The discussion reflects varying interpretations of observational data and theoretical models, with some assumptions remaining unexamined.

Who May Find This Useful

This discussion may be of interest to those exploring cosmology, the geometry of the universe, and the implications of observational data on theoretical models.

  • #31
Whitewolf4869 said:
In other words its not relevant water is water and space is space and it doesn't mater what shape the container is


Actually, it does matter quite a bit. In immediate practical terms, probably more so for a body of water than for space, since the size/shape of the container says a LOT about what you can/cannot DO in that body of water/space. It's tough to get a battleship into a bathtub for example.

Understanding the "shape" of the universe may well lead to understanding of other things of more immediate relevance.

Your point of view seems contemptuous of science.
 
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  • #32
bapowell said:
The shape and geometry of the universe are ultimately different things. For example, a flat universe could be in the shape of a flat sheet or a donut. What we actually measure with cosmological observations is the intrinsic geometry of the local universe. The best way to distinguish different intrinsic geometries is to consider whether the Euclidean postulates and their consequences hold: for example, in a flat geometry, the interior angles of a triangle sum to 180 degrees. In curved geometries, this no longer holds.

OK, thanks. I understand that. So are you saying that to say 'flat universe', one means it in terms of flat geometry, 180 deg triangles, etc ?
 
  • #33
alt said:
OK, thanks. I understand that. So are you saying that to say 'flat universe', one means it in terms of flat geometry, 180 deg triangles, etc ?
Yes, that's exactly right.
 
  • #34
Does the universe's flatness mean that non Euclidean geometry isn't important in physics?
 
  • #35
kaushik_s said:
I am a bit confused on what the current model of the universe is. some are saying it is round, while others are saying it is flat. which is true?

If the universe is flat, then is it that only some part of it is flat or the whole universe is flat?

how can we prove it theoratically and mathematically?

According to the depicted universe described in special relativity, particulary concerning the Lorentz transformations, the universe is flat with a .08 margin of deviation due to the differentiation between co-motion systems. In a difference of say, a rotational axis, certain points experience alternate rates of fluctuations to compensate for their differing inertial reference frames, specifically, when evaluating that circular system of rotation, when an side undergoes a contraction by:
L0√1-v2/c2
the radius will grant an invalid conclusion in the description of the area of a circle, namely A=∏r2, which is mathematically impossible in the Euclidean geometry of a classical universe, hence the necessitation of a curved space-time.
 
  • #36
neginf said:
Does the universe's flatness mean that non Euclidean geometry isn't important in physics?

It is flat on average over very large scales. Locally it has curvature, we call that gravity and without it the Earth wouldn't orbit the Sun so yes, non-Euclidean geometry remains important.
 
  • #37
flat or round, spherical or trumpet - does the universe have a thickness ?
is it centrally thicker like 2 cymbals placed together ? how do we know if it is symmetrical ? is it getting thinner in the centre as it expands peripherally? why should it be symmetrical - was the singularity that preceded the big bang spinning in order to give it such symmetry ?
 
  • #38
urodoc said:
flat or round, spherical or trumpet - does the universe have a thickness ?
is it centrally thicker like 2 cymbals placed together ? how do we know if it is symmetrical ? is it getting thinner in the centre as it expands peripherally? why should it be symmetrical - was the singularity that preceded the big bang spinning in order to give it such symmetry ?

Urodoc, when people speak of the shape of the universe, they are speaking of a natural curvature that spacetime has over large distances. The universe doesn't have a 'shape' in the literal since, as it has no boundary.

Keep in mind that the expansion of the universe occurs everywhere at once. There is no center or boundary. Also, the universe is symmetrical because it underwent a period called 'inflation' in it's very early history. Inflation was an enormous expansion, of unimaginable magnitudes. It essentially functioned to 'iron out' any inhomogeneities in the early universe.
 
  • #39
GeorgeDishman said:
It is flat on average over very large scales. Locally it has curvature, we call that gravity and without it the Earth wouldn't orbit the Sun so yes, non-Euclidean geometry remains important.
Mark M said:
when people speak of the shape of the universe, they are speaking of a natural curvature that spacetime has over large distances.

When people talk about the curvature of the universe, they mean the curvature of space, not the curvature of spacetime. For example, in a flat FRW universe, space is Euclidean and flat, while spacetime is neither flat nor Euclidean.
 

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