What Lies Beyond Our Observable Universe?

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    Expansion Universe
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Discussion Overview

The discussion revolves around the concept of the expansion of spacetime and the nature of galaxies within the universe. Participants explore theoretical implications, observational evidence, and the interpretation of models in general relativity, focusing on whether spacetime itself expands or if it is merely the distances between galaxies that increase.

Discussion Character

  • Debate/contested
  • Conceptual clarification
  • Technical explanation

Main Points Raised

  • Some participants question how spacetime can expand at a certain acceleration, arguing that measuring spacetime using spacetime-dependent variables is problematic.
  • Others assert that spacetime does not expand, suggesting that the distances between objects increase in specific coordinate systems, which is often referred to as the expansion of space.
  • A participant proposes that the expansion is analogous to coins on a balloon, where galaxies do not expand but remain at constant spatial coordinates while the space between them increases.
  • Another viewpoint emphasizes that galaxies cluster and merge, indicating that they do not expand at the same rate as the cosmological expansion, which is a mathematical consequence of the homogeneity and isotropy of space.
  • Some participants express skepticism about the reliance on mathematical models, suggesting that observational evidence should guide understanding of the universe's evolution.
  • There is a discussion about the formation of galaxies, with some arguing that they must have expanded to their current forms, while others highlight the role of inhomogeneities in the initial matter distribution leading to galaxy formation.

Areas of Agreement / Disagreement

Participants generally disagree on the nature of spacetime expansion and the implications of observational evidence versus mathematical models. Multiple competing views remain, with no consensus reached on the fundamental nature of expansion or the behavior of galaxies.

Contextual Notes

Participants note the complexity of the discussion, highlighting that the interpretation of spacetime and expansion may depend on specific coordinate systems and the assumptions made about the universe's structure.

Who May Find This Useful

This discussion may be of interest to those exploring cosmology, general relativity, and the observational aspects of galaxy formation and evolution.

Dragohunter
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How can the fabric of spacetime expand at a certain acceleration? Isn't speed the rate of space divided by time itself? How can you measure spacetime only using variables that are dependent on spacetime? It's like trying to measure the length of a stick using a stick."Kind of like saying an eye to see. The eye can't see unless it has a pair of eyes to see itself because it's an observer obtaining and using the eye that is doing the seeing, not the eye itself." But what really is expanding? The space in and between objects or everything in reality itself? And expanding relative to what?
 
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Spacetime does certainly not expand! In certain general relativity models spatial distances between objects, as measured using a specific coordinate chart, increase which is often called expansion of space.
 
Dragohunter said:
How can the fabric of spacetime expand at a certain acceleration? Isn't speed the rate of space divided by time itself? How can you measure spacetime only using variables that are dependent on spacetime? It's like trying to measure the length of a stick using a stick."Kind of like saying an eye to see. The eye can't see unless it has a pair of eyes to see itself because it's an observer obtaining and using the eye that is doing the seeing, not the eye itself." But what really is expanding? The space in and between objects or everything in reality itself? And expanding relative to what?
It's the space between galaxies that's expanding relative to e.g. those sticks you mentioned. Sticks don't expand. They stay the same length in local inertial frames, and that means that the proper lengths between their endpoints are constant.

Galaxies on the other hand stay at constant spatial coordinates in the specific coordinate system that MeJennifer mentioned. That, combined with the properties of that coordinate system, implies that the proper distances between galaxies are increasing.

Galaxies aren't expanding either. Well, they are, but at a rate that's much less than the cosmological expansion. That's why the expansion is often explained by suggesting that you imagine coins glued to a balloon (the coins representing galaxies). The reason why galaxies don't expand is that the large-scale expansion is a mathematical consequence of homogeneity and isotropy of space, and space isn't homogeneous or isotropic at the scale of galaxies.
 
G'day from the land of ozzzzzzzz

Fredrik said

It's the space between galaxies that's expanding relative to e.g. those sticks you mentioned. Sticks don't expand. They stay the same length in local inertial frames, and that means that the proper lengths between their endpoints are constant.

What you say and what they said is disputed. To begin with, space and time cannot change, expanded ofr contracted. The only parts that can do that is matter in its varies phases.

Galaxies on the other hand stay at constant spatial coordinates in the specific coordinate system that MeJennifer mentioned. That, combined with the properties of that coordinate system, implies that the proper distances between galaxies are increasing.

Galaxies tend to cluster and merge, observations of thousands of galaxies indicate this.

Galaxies aren't expanding either. Well, they are, but at a rate that's much less than the cosmological expansion. That's why the expansion is often explained by suggesting that you imagine coins glued to a balloon (the coins representing galaxies). The reason why galaxies don't expand is that the large-scale expansion is a mathematical consequence of homogeneity and isotropy of space, and space isn't homogeneous or isotropic at the scale of galaxies.

I think many people are lost in that ballon. Too much maths and not enough observation would put anybody off track.

You are right galaxies do not expand, once sec. How did they form? They must have expanded to that form and via observation most contract back to the centre, where black holes eject matter via jets and reform via expansion of matter.
 
Sundance said:
What you say and what they said is disputed. To begin with, space and time cannot change, expanded ofr contracted. The only parts that can do that is matter in its varies phases.
I don't understand the first sentence. I'm not sure what you mean by the second either. If you mean that spacetime doesn't change, then I agree, but it's definitely the case that if we slice up spacetime into a one-parameter family of (homogeneous and isotropic) spacelike hypersurfaces that can represent space at different times, those hypersurfaces are going to be different from each other. (They all contain a factor that's a fuction of the parameter that labels the different hypersurfaces). So "space" is changing with time.

Sundance said:
Galaxies tend to cluster and merge, observations of thousands of galaxies indicate this.
That's true, but the only relevant consequence of that (in this discussion) is that we have to look at even larger scales to see why it makes sense to describe the universe as homogeneous and isotropic.

Sundance said:
I think many people are lost in that ballon. Too much maths and not enough observation would put anybody off track.
Maybe, but it's impossible to understand the expansion without understanding FLRW solutions. A FLRW solution is what you get if you assume that space is homogeneous and isotropic. There are three of them, and they all describe an expanding universe.

Sundance said:
You are right galaxies do not expand, once sec. How did they form? They must have expanded to that form and via observation most contract back to the centre, where black holes eject matter via jets and reform via expansion of matter.
Inhomogeneities in the initial matter distribution caused the formation of stars and galaxies. In other words, small inhomogeneities led to much bigger inhomogeneities, and as the inhomogeneities grew larger, those regions of space looked less and less like a region of "space" in a FLRW spacetime. That's why they don't expand at the rate of the cosmological expansion.
 
G'day from the land of ozzzzz

Rather than trying to explain the non-expanding universe.

It is better to try to understand the formation of the stars and their varies changes.

Than trying to understand the evolution of the different forms of galaxies.

By doing that, by observation one can deduce the workings of the ongoing universe.

Lets look at the link:

Hubble sees galaxies galore
http://www.spacetelescope.org/images/html/heic0406a.html

Galaxies, galaxies everywhere - as far as the NASA/ESA Hubble Space Telescope can see. This view of nearly 10,000 galaxies is the deepest visible-light image of the cosmos. Called the Hubble Ultra Deep Field, this galaxy-studded view represents a ‘deep’ core sample of the universe, cutting across billions of light-years.

The snapshot includes galaxies of various ages, sizes, shapes, and colours. The smallest, reddest galaxies, about 100, may be among the most distant known, existing when the universe was just 800 million years old. The nearest galaxies - the larger, brighter, well-defined spirals and ellipticals - thrived about 1 billion years ago, when the cosmos was 13 billion years old.

What do you think of the information?
 
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