Estimates — True Size of the Universe?

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Discussion Overview

The discussion revolves around the estimation of the true size of the universe, distinguishing between the observable universe and the entire universe. Participants explore the implications of dark energy, the inflation period after the Big Bang, and the challenges in determining the universe's overall dimensions based on current scientific understanding.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants express confusion over the lack of a definitive "true" size of the universe, emphasizing the distinction from the observable universe.
  • One participant mentions that current measurements suggest the universe could be at least 100 times the diameter of the observable universe, but it may also be spatially infinite.
  • Another participant notes that if the universe is infinite, it has always been infinite, starting from a hot dense state.
  • There are references to three classes of solutions to the Friedman Equations: closed, flat, and open, with flat and open universes being infinite in extent.
  • One participant critiques an article claiming the universe's size, arguing that its methodology is flawed and that it leads to misleading conclusions.
  • Another participant discusses the relationship between curvature measurements and estimates of the universe's size, highlighting the imprecision in current measurements and the implications of potential curvature.

Areas of Agreement / Disagreement

Participants generally agree that the universe is larger than the observable universe and that it may be infinite, but there are competing views on the implications of curvature and the validity of certain estimates. The discussion remains unresolved regarding the exact size of the universe.

Contextual Notes

Participants note limitations in current understanding, particularly regarding the inflation period and the assumptions made in curvature measurements. The estimates discussed depend heavily on the definitions and models used, and there are unresolved mathematical steps in deriving these estimates.

  • #31
javisot said:
As Ibix says, the bread example isn't very good, but PAllen's example is brilliant. There's no contradiction between having an infinite universe and it expanding; it's a property of all spacetime.
Actually, it is only a possible property of very special spacetimes. It is a feature of geometry that is hard to visualize in a 3x1 spacetime. If you imagine the case of a 1x1 spacetime (1 spatial dimension, 1 time dimension) and closed, then you can say an expanding geometry is like the surface of a cone with the apex downward and time running upward (note, the spacetime is just the surface, and 'space' is just a circle at each time). The surface of a cylinder would be a static universe. Note how it is a feature of the geometry.

In technical terms, the question is whether the spacetime manifold admits an everywhere expanding timelike congruence. This is a rare property of manifolds. For example, it is not possible in Minkowski space (Minkowski space admits an expanding congruence - the Milne congruence - within the future light cone of an event, but it does not admit a global expanding congruence).
 
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  • #32
PAllen said:
Actually, it is only a possible property of very special spacetimes. It is a feature of geometry that is hard to visualize in a 3x1 spacetime. If you imagine the case of a 1x1 spacetime (1 spatial dimension, 1 time dimension) and closed, then you can say an expanding geometry is like the surface of a cone with the apex downward and time running upward (note, the spacetime is just the surface, and 'space' is just a circle at each time). The surface of a cylinder would be a static universe. Note how it is a feature of the geometry.

In technical terms, the question is whether the spacetime manifold admits an everywhere expanding timelike congruence. This is a rare property of manifolds. For example, it is not possible in Minkowski space (Minkowski space admits an exapnding congruence - the Milne congruence - within the future light cone of an event, but it does not admit a global expanding congruence).
(When I said it was a property of all spacetime, I didn't say it was a property of all spacetimes. We're talking specifically about an infinite, expanding universe. But it's always good to clarify that)
 
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  • #33
PAllen said:
I’ve used the following analogy to picture an infinite expanding universe. Consider the universe as an (countably) infinite collection of cubic boxes of e.g. gas (at any time you can put them together mentally to make a continuous whole). Double the side of each box, you still have the same total volume (infinite) but the density in each box has decreased by a factor of 8, and distances between reference points within each box have doubled. This process can be repeated any number of times in both directions (shrinking into the past, or expanding into thr future). At all times, volume is just infinite, but density increases without bound into the past.
Why can't one simply argue that in an infinite expanding universe the distance between any two comoving objects grows without limit?
 
  • #34
timmdeeg said:
Why can't one simply argue that in an infinite expanding universe the distance between any two comoving objects grows without limit?
You can, but many people have a hard time picturing how this is possible. My suggestion provides a way to picture this that was helpful to me and many others, over the years.
 
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