Is Our Universe Flat or Embedded on a Singularity?

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Discussion Overview

The discussion revolves around the nature of the universe's geometry, specifically whether it is flat or embedded in a singularity. Participants explore concepts related to the expansion of the universe, angular size of distant galaxies, and the implications of cosmic microwave background (CMB) observations. The conversation touches on theoretical aspects, observational limitations, and the relationship between space, time, and energy.

Discussion Character

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

Main Points Raised

  • One participant expresses confusion about the relationship between the apparent size of distant galaxies and the expansion of the universe, questioning why a galaxy 10 billion light years away appears to be half the size of one 5 billion light years away.
  • Another participant clarifies that while the volume of space increases, it does not imply that the universe was larger in the past, noting that the expansion rate has changed over time.
  • A different participant suggests that if the relationship between distance and size is not linear, then the original problem may not exist.
  • One post discusses the angular diameter distance and its behavior at different redshifts, indicating a maximum value at redshift z = 1.7.
  • Participants mention the "surface of last scattering" and its implications for observing the universe beyond a certain point, noting that other forms of observation could penetrate this limit.
  • There is a proposal about redefining 'space' to potentially allow for new observational techniques, though the meaning of this is questioned by others.
  • Another participant raises a question about the concept of 'flat space' in relation to the CMB, asking if it indicates a universe embedded in a dimensional plane or horizon.
  • Responses clarify that a flat universe is characterized by Euclidean geometry and does not imply a singularity or additional dimensions beyond the observable universe.

Areas of Agreement / Disagreement

Participants express various viewpoints on the nature of the universe's geometry and the implications of cosmic observations. There is no consensus on the interpretations of these concepts, and multiple competing views remain throughout the discussion.

Contextual Notes

Participants reference complex relationships between distance, size, and angular size that may not be straightforward due to the universe's expansion. The discussion also highlights limitations in observational techniques and the definitions of space as they relate to cosmological models.

Ganzfeld
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Here's something I can never get my head around, no matter how hard I try.

As you look out in space, you look back in time. Fine. No problems yet.

Further back in time, the universe was smaller...or at least things were closer together. Hmmm...hold on just a minute. We have a problem...at least I do and I doubt I'm the only one with it.

As you look outwards...the volume of space becomes larger, not smaller. The further out you look, the larger the apparent volume becomes for each similar increase in distance...and yet, we're told that the universe was actually much SMALLER when the light from those objects was emitted.

Now I fully understand how it would be the case that further away the expansion would appear to get greater and greater. That should solve the problem ! But...that's not the real issue. It's a bit trickier than that. My problem is that I can't square this up with the angular size of objects. If the apparent expansion increases exponentially with distance, then there oughtn't to be a linear correlation between distance and size ! In other words...a galaxy 10 billion light years away should not simply appear to be half the size of one the same size at 5 billion light years.

If the increase in expansion with distance is the answer to the 'volume' problem, then surely distant galaxies ought to appear larger than their true apparent size at that distance. Yet I've never read anything that suggests other than a linear decrease in angular size proportional to distance.
 
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Ganzfeld said:
As you look outwards...the volume of space becomes larger, not smaller.

As you look outward, the volume you see (which is a superposition of a range of time in the universe's history) becomes larger, but that certainly doesn't mean that you're looking at a time when the universe itself was larger. We don't see the entire universe at every point in its history, just the small portion of it from which light has been able to reach us.
Now I fully understand how it would be the case that further away the expansion would appear to get greater and greater.

In the recent past, the universe has been accelerating (expansion rate getting greater and greater), but in the distant past, it was decelerating. This is not the resolution to your confusion, however.
In other words...a galaxy 10 billion light years away should not simply appear to be half the size of one the same size at 5 billion light years.

Actually, you're right, it isn't. The expansion of the universe destroys the simple relationship between distance, physical size, and angular size. Only in the local universe is a linear relationship a good approximation.
 
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I think the problem is that despite having copious books on the subject I've never seen anything that suggested the relationship was anything other than linear...especially with space being generally flat...so I've just assumed that it is, and that someone would have said so if it wasn't.

If it isn't, then there isn't a problem any more.
 
The angular diameter distance [itex]d_a[/itex] is defined as the distance that relates the angular diameter of the object in the sky [itex]\theta[/itex] and the actual size of the object [itex]s[/itex], such that [itex]\theta = s / d_a[/itex] as you can read in wikipedia. In the standard cosmological model this distance has a maximum value at about redshift z = 1.7, which means that the angular diameter in sky of objects of same size at different redshifts decreases until z = 1.7 and afterwards increases. In a static space that distance is equal to the actual distance measured with rulers, [itex]d_a = d[/itex], and [itex]\theta[/itex] decreases always with distance (for objects of same size).
 
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No matter how far we look, the maximum distance we can see is limited by the maximum distance light has traveled since the Big Bang, right?
 
thiotimoline said:
No matter how far we look, the maximum distance we can see is limited by the maximum distance light has traveled since the Big Bang, right?

Almost. There's actually a "surface of last scattering" at redshift of ~1100 beyond which the universe is optically thick -- that, is opaque. Of course, if you're "observing" the universe with something other than light (like neutrinos or gravitational radiation), you can see beyond that.
 
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"There's actually a "surface of last scattering" at redshift of ~1100 beyond which the universe is optically thick -- that, is opaque."

This really intriques me. In terms of the language used to describe various aspects of the observable universe. Is it possible that what we see with optical or radio tools can be recalibrated to penetrate spectral emissions by redefining 'space' itself?
 
Orionized said:
Is it possible that what we see with optical or radio tools can be recalibrated to penetrate spectral emissions by redefining 'space' itself?

I don't know what that means. Theoretically, we can probe to very early epochs with gravitational radiation, which are fluctuations in spacetime.
 
Geometry of the CMB

SpaceTiger said:
I don't know what that means. Theoretically, we can probe to very early epochs with gravitational radiation, which are fluctuations in spacetime.

What I was thinking has to do with the concept of 'flat space' in terms of the CMB. Does the perception of 'flat space' indicate a universe imbedded on a 2 dimensional 'plane' or a 1 dimensional 'horizon' line? In other words - is our universe 'on a singularity'? Please keep in mind I only wish to understand the concept of 'space' as separate from energy and time, even though I realize that space and time are inseparable as per Einstein's relativity. Now if space is 'flat', is there another 'side'? (Put another way - is it possible that the CMB functions as a form of 'boundary' to 'flat space'?)
 
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Orionized said:
What I was thinking has to do with the concept of 'flat space' in terms of the CMB. Does the perception of 'flat space' indicate a universe imbedded on a 2 dimensional 'plane' or a 1 dimensional 'horizon' line?

No.

Orionized said:
In other words - is our universe 'on a singularity'?

No.

Orionized said:
Please keep in mind I only wish to understand the concept of 'space' as separate from energy and time, even though I realize that space and time are inseparable as per Einstein's relativity. Now if space is 'flat', is there another 'side'? (Put another way - is it possible that the CMB functions as a form of 'boundary' to 'flat space'?)

A "Flat" Universe has euclidean 3-D space. Hence the planes of a flat universe are flat, and not curved.
 

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