Where Was Dark Energy Before the Accelerated Expansion Began?

In summary: No. In fact, the "dark energy" that we know about doesn't cause expansion in any meaningful sense. It causes acceleration. That's a big difference.Dark energy is not like air, expanding and pushing things along. It is a property of space itself, and it affects the behavior of objects in space, but it doesn't push or pull like ordinary matter does. It is a property of the "fabric" of spacetime, not a substance in it.but then can't we say whenever there is negative curvature, there is very very minimum expansion (say close to distances in the Planck length)?No.
  • #1
mieral
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5
Before the period of the the accelerated expansion started about 5 billion years ago.. where was the dark energy and what was it doing. Or could it only got produced 5 billion years ago and non-existent before that?
 
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  • #2
mieral said:
Before the period of the the accelerated expansion started about 5 billion years ago.. where was the dark energy and what was it doing. Or could it only got produced 5 billion years ago and non-existent before that?
It was there and it was exerting the same force per unit volume that it is now (give or take a very small amount) ... BUT, it was not ENOUGH of a force to overcome gravity. Only about 5 to 6 Billion years ago did the expansion weaken gravitational attractions enough on cosmological scales that dark energy started being stronger than the gravitational attraction.
 
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  • #3
This excerpt from Wiki's "Metric Expansion of Space" article seems to sum it up rather well...

"According to measurements, the universe's expansion rate was decelerating until about 5 billion years ago due to the gravitational attraction of the matter content of the universe, after which time the expansion began accelerating. The source of this acceleration is currently unknown. Physicists have postulated the existence of dark energy, appearing as a cosmological constant in the simplest gravitational models as a way to explain the acceleration. According to the simplest extrapolation of the currently-favored cosmological model (known as "ΛCDM"), this acceleration becomes more dominant into the future."

Seems like the relationship between 'gravity decelerating the expansion' and 'dark energy (eventually overcoming gravity) accelerating the expansion' might be a parabolic-type function, such as a graph (time plotted against metric expansion speed) with a parent function:
f(x) = x2
Once it hits that absolute minimum point, the deceleration turns into an acceleration.
Any thoughts?
EDIT: Originally had in -(x2) by mistake. Changed to x2
 
Last edited:
  • #4
phinds said:
It was there and it was exerting the same force per unit volume that it is now (give or take a very small amount) ... BUT, it was not ENOUGH of a force to overcome gravity. Only about 5 to 6 Billion years ago did the expansion weaken gravitational attractions enough on cosmological scales that dark energy started being stronger than the gravitational attraction.

What was the proof the dark energy was there before the expansion? Anything to do with the total mass energy from the Big Bang and the expansion? Or just assuming it was there because it couldn't just appear 5 billion years ago?
 
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  • #5
mieral said:
What was the proof the dark energy was there before the expansion? Anything to do with the total mass energy from the Big Bang and the expansion? Or just assuming it was there because it couldn't just appear 5 billion years ago?
As far as I'm aware, it's the latter.
 
  • #6
It's to do with observation rather than proof.
Looking at the redshifting of distant galaxies it seems that they would have been redshifting less quickly in the distant past than they are now,
 
  • #7
mieral said:
What was the proof the dark energy was there before the expansion? Anything to do with the total mass energy from the Big Bang and the expansion? Or just assuming it was there because it couldn't just appear 5 billion years ago?
There may be some evidence from the effect of dark energy on large scale structure at relatively early times, such as the Integrated Sachs-Wolfe effect, but it's necessarily weak because the density is so low.

In the simplest model of dark energy, it is simply a cosmological constant, and a cosmological constant has a constant value at all points in space and at all times. It just wouldn't have had much effect until a few billion years ago because everything else in the universe was so much more dense until then.
 
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  • #8
I suddenly have a mental block over something. Please follow this logic:

Negative curvature is tidal gravity where things antigravitate (geodesic converge).
Dark matter expand spacetime so dark matter antigraviate.
Dark matter causes negative curvature where the metric expand?
Does it mean whenever there is negative curvature, the metric expand?
But high above the Earth where there is negative curvature.. it doesn't mean there is metric expansion.
So how do you know whether metric expansion occurs in negative curvature or there is no metric expansion and just tidal gravity??
 
  • #9
mieral said:
Negative curvature is tidal gravity where things antigravitate (geodesic converge).

No. Negative curvature means geodesics diverge. That is what dark energy (not dark matter--see below) does.

mieral said:
Dark matter expand spacetime

No. "Expand spacetime" doesn't make sense (neither does "metric expansion"). Dark matter gravitates the same way ordinary matter gravitates. That means, heuristically, that it causes positive curvature in tangential directions (geodesics falling radially inward at different angular coordinates will converge), and negative curvature in the radial direction (geodesics falling radially inward at the same angular coordinates, but starting from different radial coordinates, will diverge).

Did you mean dark energy?

The rest of your post just seems confused.
 
  • #10
PeterDonis said:
No. Negative curvature means geodesics diverge. That is what dark energy (not dark matter--see below) does.
No. "Expand spacetime" doesn't make sense (neither does "metric expansion"). Dark matter gravitates the same way ordinary matter gravitates. That means, heuristically, that it causes positive curvature in tangential directions (geodesics falling radially inward at different angular coordinates will converge), and negative curvature in the radial direction (geodesics falling radially inward at the same angular coordinates, but starting from different radial coordinates, will diverge).

Did you mean dark energy?

The rest of your post just seems confused.

I'm sorry. Yes. I meant Dark energy and incorrectly written dark matter. After thinking about it for a day. I think negative curvature doesn't automatically mean there is expansion and only in the presence of dark energy is there expansion.. right.. but then can't we say whenever there is negative curvature, there is very very minimum expansion (say close to distances in the Planck length)?

What's the right word for "metric expansion"? I thought one couldn't use "space expansion" nor "spacetime expansion"? Thank you.
 
  • #11
mieral said:
I think negative curvature doesn't automatically mean there is expansion

They are two separate concepts. Whether there is a connection between them depends on the specific spacetime. There are spacetimes that have negative curvature but no expansion; and there are spacetimes that have expansion but no negative curvature. There are also spacetimes that have both.

mieral said:
only in the presence of dark energy is there expansion

If you mean, only in the presence of dark energy is there negative curvature and expansion, that's not correct either, at least not with the usual definition of "dark energy", where it has constant density everywhere. There is a much wider range of possible models which have negative curvature and expansion, but allow the density of whatever-it-is that is causing the expansion and negative curvature to vary.

mieral said:
can't we say whenever there is negative curvature, there is very very minimum expansion (say close to distances in the Planck length)?

No. See above.

mieral said:
What's the right word for "metric expansion"?

It's better to describe the specific model you are using; general terms like this are too vague.
 
  • #12
PeterDonis said:
They are two separate concepts. Whether there is a connection between them depends on the specific spacetime. There are spacetimes that have negative curvature but no expansion; and there are spacetimes that have expansion but no negative curvature. There are also spacetimes that have both.
If you mean, only in the presence of dark energy is there negative curvature and expansion, that's not correct either, at least not with the usual definition of "dark energy", where it has constant density everywhere. There is a much wider range of possible models which have negative curvature and expansion, but allow the density of whatever-it-is that is causing the expansion and negative curvature to vary.
No. See above.
It's better to describe the specific model you are using; general terms like this are too vague.

In the Scientific American article "Misconceptions of the Big Bang" where it was supposed to correct misconceptions http://coe.kean.edu/~afonarev/Physics/ExtraCredit_files/Big bang/Big Bang-1.htm , there seems to be a misconception within:

"Renowned physicists, authors of astronomy textbooks and prominent popularizers of science have made incorrect, misleading or easily misinterpreted statements about the expansion of the universe. Because expansion is the basis of the big bang model, these misunderstandings are fundamental. Expansion is a beguilingly simple idea, but what exactly does it mean to say the universe is expanding? What does it expand into? Is Earth expanding, too? To add to the befuddlement, the expansion of the universe now seems to be accelerating, a process with truly mind-stretching consequences."
<snipped>
"This balloon analogy should not be stretched too far. From our point of view outside the balloon, the expansion of the curved two-dimensional rubber is possible only because it is embedded in three-dimensional space. Within the third dimension, the balloon has a center, and its surface expands into the surrounding air as it inflates. One might conclude that the expansion of our three-dimensional space requires the presence of a fourth dimension. But in Einstein's general theory of relativity, the foundation of modern cosmology, space is dynamic. It can expand, shrink and curve without being embedded in a higher-dimensional space."

I thought it was emphasized in physicsforums that space couldn't expand, shrink and curve.. only the metric could do that, right?

If you were to simply describe the universe expansion. What should you really use when so many phrases can't be used? I thought "metric expansion" was correct.. could "metric expands" be more correct than "metric expansion" again in describing the universe expansion?
 
  • #13
mieral said:
I thought it was emphasized in physicsforums that space couldn't expand, shrink and curve

Yes.

mieral said:
only the metric could do that

Spacetime can curve, but it can't expand or shrink. What expands or shrinks are families of worldlines.

mieral said:
What should you really use when so many phrases can't be used?

The family of worldlines describing "comoving" observers--observers who always see the universe as homogeneous and isotropic--is expanding. That means these observers are moving apart.
 
  • #14
Dark energy is assumed to have a fixed density in the universe, regardless of the scale of the universe. This is in contrast to matter and radiation, which decrease in density as the universe expands. (The matter and energy get spread out over more space, decreasing the density. Moreover, energy is also redshifted as the universe expands.) That's because dark energy isn't a material that can be spread out over space, but rather some kind of property of space itself. Probably. We really are just guessing with this dark energy business.

So in the early universe, dark energy was still present, but the matter and radiation densities were much larger and the dark energy could be ignored.
 
  • #15
PeterDonis said:
Yes.
Spacetime can curve, but it can't expand or shrink. What expands or shrinks are families of worldlines.
The family of worldlines describing "comoving" observers--observers who always see the universe as homogeneous and isotropic--is expanding. That means these observers are moving apart.

I'm reading all your justifications in PF archives why "space expand" is not correct terms. Then I came across this:
https://www.physicsforums.com/threads/spacetime-what-is-it.862012/page-4
in message #65 you wrote regarding a video shared by a poster where a professor described about the concept of space expanding or at a very specific number for the doubling of space every 10^-35/s.

certain Tionis wrote: Is the professor wrong?
you wrote: "He isn't "right" or "wrong". He's talking about an interpretation, not about the actual physics. He's not trying to give you an actual physical model that you can use to draw physical conclusions. He's just making an analogy for people who don't know the physical model and don't want one."

When you used the word "interpretation" above. Did you mean describing space as expanding was a valid interpretation like Bohmian mechanics where particles have trajectories? Is Bohmian mechanics an "actual physical model"? Or can "space expanding" not a valid interpretation at all like BM, MWI, etc.?
 
  • #16
Khashishi said:
Dark energy is assumed to have a fixed density in the universe, regardless of the scale of the universe. This is in contrast to matter and radiation, which decrease in density as the universe expands. (The matter and energy get spread out over more space, decreasing the density. Moreover, energy is also redshifted as the universe expands.) That's because dark energy isn't a material that can be spread out over space, but rather some kind of property of space itself. Probably. We really are just guessing with this dark energy business.

So in the early universe, dark energy was still present, but the matter and radiation densities were much larger and the dark energy could be ignored.

Is it a mainstream view that dark energy can either be on the left or right side of the Einstein Equations? Were you describing in on the left or right side. What happens if it is on the right side? See this for reference: https://www.physicsforums.com/threads/what-does-a-cosmological-constant-mean.798684/
 
  • #17
mieral said:
When you used the word "interpretation" above. Did you mean describing space as expanding was a valid interpretation like Bohmian mechanics where particles have trajectories?

Yes, if you also understand that I meant that neither is worth spending time thinking about, IMO. Interpretations are not physics. You can't use them to make predictions or analyze experiments. You have to first make predictions or analyze experiments using the actual physical theory--the actual math. Then, if you really feel the need, you can use an "interpretation" to make up a story after the fact about what is going on. But I don't see the point of the last part; it doesn't actually tell you anything you don't already know. But it can mislead you into thinking you know something new, which is not good.

mieral said:
Is Bohmian mechanics an "actual physical model"?

No. It's an interpretation. See above.

mieral said:
can "space expanding" not a valid interpretation at all like BM, MWI, etc.?

All of those are interpretations; I don't see the point of asking whether an interpretation is "valid" or "invalid", since all interpretations of a given physical theory (QM for BM/MWI, the FRW spacetime in cosmology for "space expanding") make the same predictions, so as far as physics is concerned they're all the same.
 
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  • #18
mieral said:
Is it a mainstream view that dark energy can either be on the left or right side of the Einstein Equations?

In the sense that there are mainstream treatments of the subject that put it on either side, yes. But any single mainstream treatment will probably put it on just one side, and might even make arguments that claim to justify that placement over the other placement.

Mathematically, there is no difference; the equation is just as valid either way.

Physically, putting dark energy on the left makes it seem like a property of spacetime, whereas putting it on the right makes it seem like a kind of stress-energy. The latter view is probably more common in recent treatments. But both versions make all of the same physical predictions, so they're not different models, they're just different ways of writing down the same model mathematically.

mieral said:
Were you describing in on the left or right side.

Everything I've said is consistent with it being on either side. Both versions make all of the same predictions. See above.
 
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  • #19
PeterDonis said:
They are two separate concepts. Whether there is a connection between them depends on the specific spacetime. There are spacetimes that have negative curvature but no expansion; and there are spacetimes that have expansion but no negative curvature. There are also spacetimes that have both.

Uhm.. what spacetime have expansion but no negative curvature??

If you mean, only in the presence of dark energy is there negative curvature and expansion, that's not correct either, at least not with the usual definition of "dark energy", where it has constant density everywhere. There is a much wider range of possible models which have negative curvature and expansion, but allow the density of whatever-it-is that is causing the expansion and negative curvature to vary.
No. See above.
It's better to describe the specific model you are using; general terms like this are too vague.
 
  • #20
There was an example in the other thread. A cone that opens up have horizontal slices circles, which get bigger as you move up. So there is space expansion but the curvature of the cone is zero.

But you need to specify what you mean by curvature. If that notion is not somewhat clear to you, then you'll only confuse yourself more.

Also it is probably not a good idea to think of curvature causing geodesics to diverge or converge. That can happen with zero curvature. Two observers moving away from each other with constant velocity will have world lines that diverge, and two observers moving towards each other will have world lines that converge. But there is no gravity nor curvature. You should think of curvature (and gravity) as related to world lines converging or diverging at an accelerated rate as oppose to at a constant rate.
 
  • #21
mieral said:
what spacetime have expansion but no negative curvature??

FRW spacetime with zero dark energy.
 
  • #22
martinbn said:
Also it is probably not a good idea to think of curvature causing geodesics to diverge or converge. That can happen with zero curvature.

To clarify, by "converge" and "diverge" I mean relative acceleration of nearby geodesics, not relative velocity. Dark energy causes nearby geodesics to accelerate away from each other; ordinary matter causes nearby geodesics (inside the matter) to accelerate towards each other. In flat spacetime, neither of those things can happen.
 
  • #23
PeterDonis said:
To clarify, by "converge" and "diverge" I mean relative acceleration of nearby geodesics, not relative velocity. Dark energy causes nearby geodesics to accelerate away from each other; ordinary matter causes nearby geodesics (inside the matter) to accelerate towards each other. In flat spacetime, neither of those things can happen.

Yes, that was the point I was trying to make. I was not sure if the OP realized that.
 
  • #24
PeterDonis said:
Yes, if you also understand that I meant that neither is worth spending time thinking about, IMO. Interpretations are not physics. You can't use them to make predictions or analyze experiments. You have to first make predictions or analyze experiments using the actual physical theory--the actual math. Then, if you really feel the need, you can use an "interpretation" to make up a story after the fact about what is going on. But I don't see the point of the last part; it doesn't actually tell you anything you don't already know. But it can mislead you into thinking you know something new, which is not good.

So you are saying to talk to laymen quickly... It's indeed not wrong to say "space expands". Like if you want to make speeches in front of town assembly and you want to make them get the idea their Newtonian mindset was already outdated by many centuries and they must get more open minded and say for example science nowadays is so liberated and we have such things as "space expands".

Also I need to know what is the official interpretations of Spacetime called. In Quantum Mechanics, we have Bohmian Mechanics, MWI, Objective Collapse, TI, Copenhagen. In Spacetime, what are the official names, anyone? Note I won't focus on this as I know how much you and others may hate interpretations. But I just want to know the official names of Spacetime interpretations so I can google them (and don't worry won't discuss them here). Thanks.
No. It's an interpretation. See above.
All of those are interpretations; I don't see the point of asking whether an interpretation is "valid" or "invalid", since all interpretations of a given physical theory (QM for BM/MWI, the FRW spacetime in cosmology for "space expanding") make the same predictions, so as far as physics is concerned they're all the same.
 
  • #25
mieral said:
So you are saying to talk to laymen quickly... It's indeed not wrong to say "space expands".

Not if you don't mind correcting them as soon as they start to make erroneous inferences from that statement. Which they will do very quickly. We have many, many threads here on PF that attest to that.

mieral said:
Also I need to know what is the official interpretations of Spacetime called

The two most common interpretations of GR are the curved spacetime interpretation, and the "spin-2 field in flat spacetime" interpretation.
 
  • #26
PeterDonis said:
Not if you don't mind correcting them as soon as they start to make erroneous inferences from that statement. Which they will do very quickly. We have many, many threads here on PF that attest to that.
Why, when one wants to share quantum mechanics with layman.. is it not possible to start by sharing them about Bohmian Mechanics? A person I initially shared it said of course particles had trajectories. I countered by telling him there was no trajectories.. but on second thought I remembered BM mentioning there was trajectories. So Is there something wrong by sharing with laymen directly BM and saying there were trajectories?

How does the above differs to sharing them about space being able to expand? Like it's ok to share with laymen about Bohmian Mechanics initially and yet not about spaceing expansion. Is it because Bohmian Mechanics are more advanced in their formalism than this space expansion interpretation? If they have same level of sophistication.. why one can share BM initally and not space able to expand?

The two most common interpretations of GR are the curved spacetime interpretation, and the "spin-2 field in flat spacetime" interpretation.

I'm very familiar with this "spin-2 field in flat spacetime" having a book that described it. But what's this "curved spacetime interpretation" you talked about.. what's the other name since in standard General Relativity, it is curved spacetime too.
 
  • #27
mieral said:
Why, when one wants to share quantum mechanics with layman.. is it not possible to start by sharing them about Bohmian Mechanics?

Of course it's possible to do this. You can tell people whatever you want. I just don't think it's a good idea. I don't think it's a good idea to start with any interpretation. You should start with the actual physics: what model we use to make predictions, what we actually observe, and how the two match up.

That way you are sure you're not telling people anything they will have to unlearn, and you're not telling them anything they can use to make erroneous inferences. As soon as you go beyond that into an interpretation, those things are no longer true.

Experts in the field use interpretations to communicate with each other because they know their limitations. They don't use them to actually make predictions. They use them in order to have handy shorthand in ordinary language for things where all the other experts they're talking to know the underlying mathematical model and what the ordinary language terms in the interpretation refer to in that model. But this only works because everybody knows all those things, so they aren't being misled.

Occasionally, you find an expert who is able to use interpretations to communicate with lay people without misleading them, but it's rare. Feynman comes to mind as an example: if you read one of his pop science books, such as QED: The Strange Theory of Light and Matter, or The Character of Physical Law, you will find him using interpretations (though sparingly), but you will also find him constantly cautioning about the things he is leaving out and not to take what he is saying too literally. Most scientists who do pop science, however, are not that careful.

Similar comments apply to the "space expanding" interpretation of cosmological models.

mieral said:
in standard General Relativity, it is curved spacetime too

Not really. Curved spacetime is actually an interpretation. It's just so common that it's the one that is almost always used in textbooks and papers to describe things in words, so it has filtered down into pop science books on the subject as though it were the actual theory. But the underlying math of GR does not have to be interpreted as curved spacetime; that should be evident since, as you agree, there is another interpretation, the spin-2 field in flat spacetime interpretation, of the same math. Most GR textbooks talk about this, although not many spend a lot of time on the spin-2 field interpretation (Weinberg's book, as I understand it, is an exception; I don't have it so I can't say from my own experience.)

For an example of a pop science book that actually explains this in connection with GR, try Kip Thorne's Black Holes and Time Warps. (Thorne also mentions a third interpretation, which he calls the "membrane paradigm", but it's not really a complete interpretation of GR because it doesn't use the same math, it only uses an approximation that's valid in some cases but not all.) But again, for a pop science book to go to that trouble is rare.
 
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  • #28
PeterDonis said:
Of course it's possible to do this. You can tell people whatever you want. I just don't think it's a good idea. I don't think it's a good idea to start with any interpretation. You should start with the actual physics: what model we use to make predictions, what we actually observe, and how the two match up.

That way you are sure you're not telling people anything they will have to unlearn, and you're not telling them anything they can use to make erroneous inferences. As soon as you go beyond that into an interpretation, those things are no longer true.

Experts in the field use interpretations to communicate with each other because they know their limitations. They don't use them to actually make predictions. They use them in order to have handy shorthand in ordinary language for things where all the other experts they're talking to know the underlying mathematical model and what the ordinary language terms in the interpretation refer to in that model. But this only works because everybody knows all those things, so they aren't being misled.

Occasionally, you find an expert who is able to use interpretations to communicate with lay people without misleading them, but it's rare. Feynman comes to mind as an example: if you read one of his pop science books, such as QED: The Strange Theory of Light and Matter, or The Character of Physical Law, you will find him using interpretations (though sparingly), but you will also find him constantly cautioning about the things he is leaving out and not to take what he is saying too literally. Most scientists who do pop science, however, are not that careful.

Similar comments apply to the "space expanding" interpretation of cosmological models.
Not really. Curved spacetime is actually an interpretation. It's just so common that it's the one that is almost always used in textbooks and papers to describe things in words, so it has filtered down into pop science books on the subject as though it were the actual theory. But the underlying math of GR does not have to be interpreted as curved spacetime; that should be evident since, as you agree, there is another interpretation, the spin-2 field in flat spacetime interpretation, of the same math. Most GR textbooks talk about this, although not many spend a lot of time on the spin-2 field interpretation (Weinberg's book, as I understand it, is an exception; I don't have it so I can't say from my own experience.)

For an example of a pop science book that actually explains this in connection with GR, try Kip Thorne's Black Holes and Time Warps. (Thorne also mentions a third interpretation, which he calls the "membrane paradigm", but it's not really a complete interpretation of GR because it doesn't use the same math, it only uses an approximation that's valid in some cases but not all.) But again, for a pop science book to go to that trouble is rare.

Thank you for these masterpiece explanations. I've often been thinking of it. So the math of GR and QM are the Maps and the real world is the Territory. And they mentioned not to mistaken the Map for the Territory. But is there anything (other examples) in physics where the Map is itself the Territory? For example in computer programs.. there are only maps, no territory. If our reality are like programs and the GR and QM maths are the only thing that exist because we are inside some kind of program. Then can we say only Maps exist and they are the Terrority themselves? Or is the Big Bang computer software and simulation package called the Terrority and the math of GR and QM the Maps? Or all just maps? Thank you!
 
  • #29
mieral said:
is there anything (other examples) in physics where the Map is itself the Territory?

No.

mieral said:
in computer programs.. there are only maps, no territory

How much computer programming have you done? Any program that interacts with the rest of the world (which is any program that's at all interesting) has a territory (the rest of the world) which is not the same as the map (whatever internal representations the program uses to determine how it interacts with the rest of the world).

The rest of your post just seems to build on this basic confusion.
 
  • #30
This thread is veering off into personal speculation and is now closed.
 

1. Where did dark energy come from?

The origin of dark energy is still a mystery to scientists. Some theories suggest that it has been present since the beginning of the universe, while others propose that it is a result of the interactions between particles in the vacuum of space.

2. Was dark energy always present?

It is believed that dark energy has always been present, but its effects were not noticeable until about 5 billion years ago when the expansion of the universe began to accelerate.

3. How do we know dark energy was not present before the accelerated expansion?

Scientists have observed the expansion of the universe using various methods, such as measuring the distance and brightness of distant supernovae. These observations have shown that the expansion of the universe was decelerating until about 5 billion years ago, indicating that dark energy was not present before then.

4. What caused the accelerated expansion to begin?

The exact cause of the accelerated expansion is still unknown. However, many scientists believe that it is due to the presence of dark energy, which has a repulsive effect on matter and causes the expansion to accelerate.

5. Will dark energy continue to cause the expansion of the universe to accelerate?

Based on current observations, it is believed that dark energy will continue to cause the expansion of the universe to accelerate. However, the rate of acceleration may change over time, depending on the amount and properties of dark energy.

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