Dark Energy & Expanding Universe: Newtonian Perspective

In summary, the observable universe is expanding, but we don't know how much farther it will go. There may be more matter out there that we haven't seen yet, and general relativity still applies.
  • #1
darkside00
83
0
A very simple way to explain the observable universe expanding:
Perhaps there is just a bunch of matter surrounding the observable universe and all the observable stars/galaxies are moving per the gravitational field created by matter outside that we have not yet seen. Thoughts?
 
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  • #2
A uniform spherical shell of matter exerts a net gravitational force of zero on any object inside it:

https://www.physicsforums.com/showthread.php?t=121120

Considering that, how would you distribute your "outside" matter so as to produce a net outward force on all the "inside" matter?
 
  • #3
The outside matter could be distributed to pull the star/galaxies away as we see it. Just cause we haven't seen all matter yet, we can't get zero
 
  • #4
jtbell said:
A uniform spherical shell of matter exerts a net gravitational force of zero on any object inside it:

https://www.physicsforums.com/showthread.php?t=121120

Considering that, how would you distribute your "outside" matter so as to produce a net outward force on all the "inside" matter?

It's clear this is true of Newtonian gravity. Is it clear that this still holds in an expanding universe that obeys general relativity?
 
  • #5
Is it clear that this still holds in an expanding universe that obeys general relativity?
Yes, that's proven.
 
  • #6
phyzguy said:
It's clear this is true of Newtonian gravity. Is it clear that this still holds in an expanding universe that obeys general relativity?
Ich said:
Yes, that's proven.

On the other hand, how do we know that the area outside the observable universe obeys general relativity?
 
  • #7
On the other hand, how do we know that the area outside the observable universe obeys general relativity?
That was not the question.
 
  • #8
yeah, the question is does this outside matter affect our universe(if it exists without us seeing), off course it does
 
  • #9
Or are we certain we've seen all matter? to make the net zero.
perhaps matter outside 'not our observable" is moving opposite direction
 
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  • #10
Er, no. jtbell already explained why this does not work. Furthermore, we see distant galaxies [the ones receeding the 'fastest'] as they were billions of years ago, so it us, not them, that is closest to this hypothetical unseen matter surrounding the observable universe. Apparently no one notified the Andromeda galaxy because it is on a collision course with the Milky Way.
 
  • #11
Could the outside matter's distribution be determined by where matter would most likely agglomerate in multiverses? I assume we have not seen all matter since any dark matter outside our line of sight to another observable galaxy/object would be difficult to detect.
 
  • #12
darkside00 said:
A very simple way to explain the observable universe expanding:
Perhaps there is just a bunch of matter surrounding the observable universe and all the observable stars/galaxies are moving per the gravitational field created by matter outside that we have not yet seen. Thoughts?

but if there is already matter outside the observable universe that means tha the Universe is not expanding only the amount of the Universe we can actually see is increasing. also does that mean that there is a finite point to which te Universe can expand??
 

1. What is dark energy?

Dark energy is a hypothetical form of energy that is thought to make up about 70% of the total mass-energy of the universe. It is believed to be responsible for causing the expansion of the universe to accelerate.

2. How does dark energy affect the expansion of the universe?

Dark energy is believed to have a repulsive gravitational effect, causing the expansion of the universe to accelerate. This means that the space between galaxies is constantly increasing, leading to a larger and more spread out universe over time.

3. How was dark energy discovered?

Dark energy was first hypothesized by Albert Einstein in his theory of general relativity. It was later observed in the late 1990s through studies of distant supernovae, which showed that the expansion of the universe was accelerating rather than slowing down as previously thought.

4. What is the Newtonian perspective on dark energy?

The Newtonian perspective on dark energy is that it can be explained through the concept of the cosmological constant, which was first introduced by Newton as a way to explain the stability of the universe. This constant is now thought to represent the density of dark energy in the universe.

5. How does dark energy fit into our current understanding of the universe?

Dark energy is a fundamental component of the current model of the universe, known as the Lambda-CDM model. This model also includes dark matter, which makes up about 25% of the total mass-energy of the universe, and ordinary matter, which makes up the remaining 5%. Together, these components help us explain the structure and evolution of the universe.

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