Expansion rate of the universe

In summary, the current understanding of the expanding universe is that it is constantly increasing in size, with the expansion rate possibly changing over time. This is determined by observing the recession rate of nearby galaxies and objects at different points in time. There are different theories about the future of the universe, with the currently favored model predicting a continuous expansion. The idea of time reversal and time dilation is taken into consideration when interpreting observations, but it does not affect our subjective experience of time. The concept of a cosmological constant was introduced by Einstein to explain why the universe does not collapse due to gravity, but it was later abandoned in favor of the expanding universe model. The reason for the expansion of the universe is still not fully understood, but it is currently
  • #1
salhuneidi
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I am not an expert on this matter but it got really interested in the physics of the expanding universe, I believe that the universe is expanding. My question is how could science know if this expansion rate is increasing or decreasing, and how can science ever measure such a rate.
Also I would like to know what science says about the idea of the universe contracting.
 
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  • #2
salhuneidi said:
I am not an expert on this matter but it got really interested in the physics of the expanding universe, I believe that the universe is expanding. My question is how could science know if this expansion rate is increasing or decreasing, and how can science ever measure such a rate.

Remember that the more distant the galaxy or quasar we're looking at, the further we're looking back in time. The recession rate of nearby galaxies give us an idea of the current expansion rate because we're not looking very far back in time (relative to the age of the universe) when we look at them. On the other hand, when I look at a galaxy with a redshift of 1 or 2, I'm looking at it when the universe was much younger and had a different expansion rate.


Also I would like to know what science says about the idea of the universe contracting.

The universe might contract in the future, but it's hard to say. The favorite model at the moment has it expanding indefinitely (at an ever increasing rate), but there are other models that fit the data which predict a coming contraction phase.
 
  • #3
Thanks spacetiger, I am also wondering that when the expansion rate increases doesn't this mean that all time is actually faster, and isn't time related somehow to the expansion rate.
I just need a little more info about how time is affected by the expansion and the rate of expansion and it would be great if you can direct me to some resources about these topics.
I am also interested in the idea of time reversal as a result of universe contraction, and if there is any information out there about this topic it would be great.
 
  • #4
salhuneidi said:
Thanks spacetiger, I am also wondering that when the expansion rate increases doesn't this mean that all time is actually faster, and isn't time related somehow to the expansion rate.

Cosmic time is defined by the clock of an observer at rest with respect to the Hubble flow or CMB. There is a relative time dilation between us and the distant galaxy (and it's considered when interpreting the observations), but we wouldn't experience time any differently now than 10 billion years ago.
 
  • #5
General relativity is the short answer. Distant [high z] objects age more slowly than more nearby objects from our point of view. Sandard candles [i.e., supernova] is what convinced most scientists exansion started accelerating a while back. Figuring out why is a horse of a different color.
 
  • #6
Fine, but can one explain WHY is the universe EXPANDING?
 
  • #7
When Einstein worked out his field equations, he realized his model of the universe was unstable. Thus, he added the 'cosmological constant' to force a steady state universe [which as all the rage in those days]. But he quickly realized this was an untenable solution. His steady state universe was literally balanced upon the point of his pencil. He cheerfully abandoned that idea when Hubble found evidence the universe was exanding. Although Hubble was never entirely satisfied with that conclusion, current evidence suggests he was correct.
 
  • #8
Chronos said:
When Einstein worked out his field equations, he realized his model of the universe was unstable. Thus, he added the 'cosmological constant' to force a steady state universe [which as all the rage in those days]. But he quickly realized this was an untenable solution. His steady state universe was literally balanced upon the point of his pencil. He cheerfully abandoned that idea when Hubble found evidence the universe was exanding. Although Hubble was never entirely satisfied with that conclusion, current evidence suggests he was correct.

So, is it the cosmological constant the reason of expansion? If yes, what is than the cosmological constant?
 
  • #9
If I'm right, the cosmological constant was introduced to oppose the rate of expansion exactly opposite - so the universe was in this steady, non-expanding or contracting, state.

I think what you are after is the Hubble constant, which is the rate the universe is expanding at. But I believe that is just a value and I'm not sure how or why the universe is expanding at such a speed.

[Please don't be harsh if I'm wrong...I've only currently started to take up my own learning of this subject as my school doesn't tell me anything about it!]
 
  • #10
The)End)Of)The)World said:
If I'm right, the cosmological constant was introduced to oppose the rate of expansion exactly opposite - so the universe was in this steady, non-expanding or contracting, state.

I think what you are after is the Hubble constant, which is the rate the universe is expanding at. But I believe that is just a value and I'm not sure how or why the universe is expanding at such a speed.

[Please don't be harsh if I'm wrong...I've only currently started to take up my own learning of this subject as my school doesn't tell me anything about it!]
Welcome to PF, TEOTW! I think you grasp the essentials. Einstein's motivation for inserting the CC was to explain why the universe does not collapse. Like Newton, he realized gravity posed a serious problem in an infinitely old universe.
 
  • #11
Could the Universe be expanding simply because it is in a giant vacuum? When the universe was an infinitely small point. It was in some sort of space. A giant void? Infinite void? So after the BB the Universe is steadily expanding to fill the vacuum of the void. So then wouldn't it expand faster as it went because as matter pulls apart there is less gravitational pull between the matter. So there becomes less and less force slowing down the expansion?
 
  • #12
UglyEd said:
Could the Universe be expanding simply because it is in a giant vacuum? When the universe was an infinitely small point. It was in some sort of space. A giant void? Infinite void? So after the BB the Universe is steadily expanding to fill the vacuum of the void. So then wouldn't it expand faster as it went because as matter pulls apart there is less gravitational pull between the matter. So there becomes less and less force slowing down the expansion?

Not quite. A vacuum would also be considered part of the universe. It is very ahrd to grasp logically, but essentially what happens is that it just expands, it doesn't expand into some space or into a void, it just expands.
 
  • #13
it just expands, it doesn't expand into some space or into a void, it just expands.

How do we know this? How do we know that what we consider to be the universe. Isnt just an explosion in a great void. The universe is steadily expanding and taking up more and more space (area) what space is it taking up?
 
  • #14
GR describes the expansion internally to the universe itself, within the fabric of space-tme. Empty space (the void?) itself expands. Objects within the universe move further apart, even if the universe is infinite in extent. We can say nothing about what happens beyond the universe, or though there are conjectures that other universes may exist.

Garth
 
  • #15
The second law of thermodynamics says that a system will move from order to disorder. In the case of the expansion of the universe if a quantity of matter is surrounded by nothing it will expand to fill the void, unless it has sufficient gravity to haul itself into a single lump. Because we don't really know the size of the universe we cannot really ascertain if it will expand forever or collapse. The consensus is that there is not enough gravity to collapse the universe, but there are enough mysteries to be solved that there may yet be something we have not discovered that might totally change this view.
 
  • #16
Tzemach said:
The second law of thermodynamics says that a system will move from order to disorder. In the case of the expansion of the universe if a quantity of matter is surrounded by nothing it will expand to fill the void, unless it has sufficient gravity to haul itself into a single lump. Because we don't really know the size of the universe we cannot really ascertain if it will expand forever or collapse. The consensus is that there is not enough gravity to collapse the universe, but there are enough mysteries to be solved that there may yet be something we have not discovered that might totally change this view.
Welcome to these Forums Tzemach!

The second law certainly applies to a closed system, whether the whole universe constitutes such a system or not is debatable.

The expansion of the universe may itself be increasing the total number of states available and thus explain where order has come from.

The standard understanding is that the universe of matter is not increasing in a vacuum, but that rather the vacuum in which the matter is situated is increasing in volume.

The latest results from WMAP3 suggest that, if anything, there is enough total energy-density in the universe for its gravitation to 'close' the universe. However, this requires 23% to be unknown Dark Matter and another 73% to be even more unknown Dark Energy.

Whether the universe will recollapse or not depends not only on the density but also on how that DE behaves.

Garth
 
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  • #17
The standard understanding is that the universe of matter is not increasing in a vacuum, but that rather the vacuum in which the matter is situated is increasing in volume.

Does it depend on what someone considers the Universe to be?

To make this less confusing I will make up a couple terms.

SMALL UNIVERSE= All matter was in an infinitely small space then exploded and started expanding. So that the Universe is steadily getting bigger, as the explosion/matter expands. Basically the Small Universe is just the space that the explosion from the BB is taking up. There is nothing beyond that. This is what is generally concidered "The Universe" right?

Big Universe= Or is "The Universe" the explosion and also everything beyond the space the explosion/matter is taking up? So that if we had the ability we could fly out of the explosion and beyond all matter. Into a great empty void that has no matter at all. Like as if the Small Universe was just a firecracker exploding inside a vacuum ( The Big Universe).

How could we prove either one is true or not?

To me it seems to be more likely that the Small Universe (what is I think generally concidered "The Universe") is just an explosion inside of a giant vacuum "The Big Universe". That would more easily explain why the matter from the BB is accelerating. It is expanding to fill the void. As it expands matter spreads out, thus having less and less gravitational attraction to other matter. So having less and less resistance to the expansion to fill the void/vacuum. So that would mean that the Universe will continue to expand forever.

If the universe is just the area that the BB explosion is taking up( The Small Universe). Then you have to add in hypothetical things like dark matter to explain the accelerating expansion of the Universe.

What do you think?
 
  • #18
The modern (post 1915) theory of cosmology is based on General Relativity. General Relativity describes how the space-time continuum itself is shaped by matter and energy.

When applied to the cosmological solution in which the distribution of matter and energy is isotropic and homogeneous, GR predicts expanding or contracting space. Hubble's discovery of the (nearly) linear relationship between the distance and red shift of galaxies is accepted as evidence that the universe is actually expanding, thus confirming that prediction of GR.

The theory predicts that, within a 'block' space-time, the hyper-surfaces of space expand as time progresses. This means that if we consider dust particles suspended in a vacuum, representative of the galaxies in the cosmos, then my statement
the vacuum in which the matter is situated is increasing in volume
means the dust particles all move away from each other, the whole volume expands over time.

I hope this helps,

Garth
 
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  • #19
Another way to say my theory is that. Maybe the Universe always existed. Just all the matter in it was compressed into an infinitely or very small space. With the BB the matter exploded out, and continues to expand to fill the void it is in. So what is normally thought of as the Universe is just the area the matter from the BB is taking up. But really the Universe is much larger than that. We could see the distant matter at the edge of the explosion, but there would be nothing to see beyond that. Because beyond that is just an empty void. Is there any reason that this couldn't be true?
 
  • #20
We certainly cannot be sure about what we cannot see, lying beyond our particle horizon.

I was just questionning your idea of the matter in the universe expanding into a void. If by void you mean empty space beyond the matter universe then I was pointing out in GR it is the space itself that expands and carries the matter with it.

As far as we can see the universe is more or less isotropic and homogeneous. - No really big lumps!

Garth
 
  • #21
Do we know if universe has expanded since BB or contracted anytime?
Or for how long has it been accelerating?

Thanks

:)
 
  • #22
The cosmological constant was introduced to force a static solution to Einstein's field equations. Hubble made the empirical discovery that the universe is expanding, and the Hubble constant was originally defined as simply the experimental proportionality constant between the distance and overall velocity of recession of other galaxies (not to be confused with "peculiar motion" where galaxies can be moving toward each other due to mutual gravitational attraction). GR is just a theory, but that theory DEFINES our universe as a particular solution of the equations -- there is nothing else that it is expanding in to.

As to the increased rate of expansion, the underlying is cause is not even close to being understood. Take a look at the February 2004 issue of Scientific American. The present value of the Hubble constant is based on relatively nearby galaxies, and the predicted distance based on this can be compared with the measured distance of very distant galaxies which would be a measure of the Hubble constant at a much earlier time.

Also, on http://arxiv.org (click on Form Interface, select astro-ph, and type in the number) take a look at astro-ph/0310808 for a good article on common misconceptions in cosmology. The possibility of multiverses is discussed in the May 2003 SciAm article by Max Tegmark, as well as in his article at astro-ph/0302131. I don't know how much math and physics you know, but another great source for inflationary cosmology info at a reasonable level is Watson's lectures at astro-ph/0005003. You might also get a copy of the very readable intro text by Barbara Ryden "Intro to Cosmology."
 
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1. What is the expansion rate of the universe?

The expansion rate of the universe is a measure of how fast the universe is expanding. It is typically expressed in units of kilometers per second per megaparsec (km/s/Mpc).

2. How is the expansion rate of the universe measured?

The expansion rate of the universe is measured using a variety of methods, including measuring the redshift of distant galaxies, the cosmic microwave background radiation, and the brightness of supernovae. These methods all provide consistent results and have been used to refine our understanding of the expansion rate over time.

3. Has the expansion rate of the universe always been the same?

No, the expansion rate of the universe has not always been the same. In fact, it is currently accelerating, meaning that the universe is expanding at an increasing rate. This acceleration is thought to be caused by dark energy, a mysterious force that makes up about 68% of the total energy of the universe.

4. How does the expansion rate of the universe affect the formation of galaxies?

The expansion rate of the universe has a significant impact on the formation of galaxies. As the universe expands, it becomes less dense and the gravitational pull between galaxies weakens. This allows galaxies to form and evolve over time. The rate of expansion also affects the distribution of matter in the universe, influencing the size and shape of galaxies.

5. Can the expansion rate of the universe change in the future?

While the expansion rate of the universe is currently accelerating, it is possible that it could change in the future. The exact behavior of the expansion rate is dependent on the amount and nature of dark energy in the universe, which is still not fully understood. Further research and observations will help us better understand the potential changes in the expansion rate of the universe.

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