Curvature of Space - Is it Still Relevant in Modern Physics?

Click For Summary

Discussion Overview

The discussion revolves around the relevance of the curvature of space in modern physics, particularly in the context of cosmology. Participants explore concepts related to the topology of the universe, the implications of curvature on the fate of the universe, and the relationship between curvature and the Big Crunch scenario.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants reference the idea that if one travels in a straight line in a curved space, they could eventually return to their starting point, suggesting a closed topology.
  • There is a distinction made between the concepts of topology and curvature, with some arguing that the question of whether the universe is closed or open remains unsettled.
  • One participant notes that current observations suggest the universe is flat or open, with a general consensus that the universe is either flat or open rather than closed.
  • Another participant mentions that the fate of the universe is influenced by its curvature, particularly in relation to mass density and dark energy, indicating that a closed universe could still expand indefinitely under certain conditions.
  • A study mentioned by a participant indicates that no paired circles were found in the Cosmic Microwave Background (CMB), which supports the idea of a flat universe.

Areas of Agreement / Disagreement

Participants express differing views on the current understanding of the universe's curvature and topology. While some suggest a consensus on the universe being flat or open, others maintain that the question of a closed universe is still an open topic of debate.

Contextual Notes

There are unresolved assumptions regarding the implications of dark energy on the curvature and fate of the universe, as well as the definitions of closed, flat, and open universes. The relationship between curvature and the universe's fate is also noted to be complex and dependent on various factors.

DaveC426913
Gold Member
2025 Award
Messages
24,549
Reaction score
8,866
I have not been keeping up on current cosmology theory.

Once was said that if you flew your "Spaceship of the Mind" X billion light years "thataway", and didn't stop or turn, you eventually would find yourself back where you started. The idea here is that 3-dimensional space is actually curved through a 4th dimension so that it wraps upon itself.

Is this still the prevailing notion of modern physics?



In an only loosely-related question: Is this the same curvature of 3D space upon which the eventual Big Crunch depends? i.e. if space is flat, the universe will expand forever. (I think these two questions are unrelated, despite their overlap of terms.)
 
Astronomy news on Phys.org
DaveC426913 said:
I have not been keeping up on current cosmology theory.
That's not necessarily a bad thing! :rolleyes: Just joking, but cosmology is very much a flavor-of-the-month prospect in some regards.

DaveC426913 said:
Once was said that if you flew your "Spaceship of the Mind" X billion light years "thataway", and didn't stop or turn, you eventually would find yourself back where you started. The idea here is that 3-dimensional space is actually curved through a 4th dimension so that it wraps upon itself.

Is this still the prevailing notion of modern physics?

In an only loosely-related question: Is this the same curvature of 3D space upon which the eventual Big Crunch depends? i.e. if space is flat, the universe will expand forever. (I think these two questions are unrelated, despite their overlap of terms.)
OK, you have two different concepts going here, and you realize that, so it'll be easy for you to sort them out. First off, if you can head out in one direction and come back on yourself from the opposite direction, you are in a universe that has a topology that is closed, like a sphere, a torus, or a moebius strip, etc.

The question of curvature concerns the fate of the universe, as you have accurately determined. If we are in a Big Bang universe, and the universe has a positive curvature (like a ball), the expansion of the universe will eventually slow and collapse back upon itself (closed universe). If the universe is has no curvature, it will continue expanding forever, gradually slowing, but not collapsing (flat universe). If the universe has negative curvature, it will simply continue expanding forever (open universe).
 
"...you are in a universe that has a topology that is closed, like a sphere, a torus, or a moebius strip, etc. ..."

Yup, this was the heart of my question (the other bit was a tangent).

So, is the current prevailing theory that we live in a closed universe? That we would eventually come back to our starting point? Or is this even theory at all, as opposed to conjecture?
 
DaveC426913 said:
"...you are in a universe that has a topology that is closed, like a sphere, a torus, or a moebius strip, etc. ..."

Yup, this was the heart of my question (the other bit was a tangent).

So, is the current prevailing theory that we live in a closed universe? That we would eventually come back to our starting point? Or is this even theory at all, as opposed to conjecture?
Topology is an open question for most people, and the thought that you might come back upon yourself from the opposite direction is not that widely accepted.

The "curvature" question, which can simply be equated to "is there enough mass in the universe to make it collapse back in onto itself" is more widely viewed as settled, in that most folks think the universe is either flat or open.

There are folks like myself that think the Big Bang theory is not a proper model of the universe. We are in the minority at this point, but the revolution is coming.
 
In a flat universe, as current measures indicate, the universe is spatially infinite.
 
The current observations indicate that space is almost flat (zero curvature). There are lots of geometries which fit with the requirement of zero curvature of space. The most trivial one is an infinite space R^3, but a 3-cylinder or a 3-torus inside a four dimensional spacetime can have also a flat metric on it.

This is indeed the curvature on which the fate of the universe depends, if you consider only a classical content (no dark energy). Otherwise (with dark energy), there is no direct relation between curvature and fate of the universe (a closed universe may expand forever, if it contains enough dark energy).
 
In the Issue of May of Physical Review Letters of this year there was a study searching for paired circles in the CMB, that is, to see the same configuration in opposite sides. No such paired circles were found, this is a great support for the idea that space is flat
 
Thanks meteor, I recall that paper. For a link see:
http://www.aip.org/pnu/2004/split/685-1.html
 
Last edited by a moderator:

Similar threads

  • · Replies 25 ·
Replies
25
Views
4K
  • · Replies 12 ·
Replies
12
Views
7K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 1 ·
Replies
1
Views
6K
  • · Replies 4 ·
Replies
4
Views
1K
  • · Replies 11 ·
Replies
11
Views
4K
  • · Replies 0 ·
Replies
0
Views
4K
  • · Replies 21 ·
Replies
21
Views
7K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 9 ·
Replies
9
Views
3K