What Lies Beyond Our Observable Universe?

In summary, the conversation discusses the concept of the expansion of spacetime and the difficulties of measuring it using only variables dependent on spacetime. It also explores the idea of galaxies and their formation, and how they are not expanding at the same rate as the overall expansion of the universe. The conversation delves into the mathematical concepts of FLRW solutions and the homogeneity and isotropy of space, ultimately leading to a better understanding of the evolution of galaxies and the non-expanding nature of the universe.
  • #1
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 dependant 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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  • #2
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.
 
  • #3
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 dependant 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.
 
  • #4
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.
 
  • #5
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.
 
  • #6
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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FAQ: What Lies Beyond Our Observable Universe?

What is the expansion of the universe?

The expansion of the universe refers to the observed phenomenon that the distance between galaxies is increasing over time. This means that the universe is expanding, rather than being a static or contracting entity.

How do scientists measure the expansion of the universe?

Scientists use a variety of techniques to measure the expansion of the universe, including the redshift of light from distant galaxies, the Hubble constant, and the cosmic microwave background radiation. These methods provide evidence for the accelerating expansion of the universe.

What is dark energy and how does it relate to the expansion of the universe?

Dark energy is a mysterious force that is thought to be responsible for the accelerating expansion of the universe. It is believed to make up about 70% of the total energy in the universe and its effects can be seen in the expansion rate of the universe.

What does the expansion of the universe mean for the future of our universe?

The expansion of the universe is currently accelerating, which means that the distance between galaxies will continue to increase. This will eventually lead to the "heat death" of the universe, where all matter and energy are evenly distributed and no more work can be done.

Is the expansion of the universe affected by the presence of matter and dark matter?

Yes, both matter and dark matter play a role in the expansion of the universe. Matter has a gravitational pull that can slow down the expansion, while dark matter's gravitational effects can accelerate it. However, dark energy is still the dominant force driving the expansion.

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