What Could Cause a Big Crunch in the Expansion of the Universe?

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Discussion Overview

The discussion revolves around the concept of the Big Crunch and the factors influencing the expansion of the universe, particularly in relation to dark energy and gravity. Participants explore theoretical implications, the role of different types of matter, and the dynamics of cosmic expansion.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants suggest that if the universe is expanding, its increasing volume leads to decreasing density and gravitational force, potentially accelerating expansion.
  • Others argue that gravity acts to decelerate expansion, and that the observed acceleration is attributed to dark energy, which is not fully understood.
  • A participant explains that the original expansion from the Big Bang is slowed by gravity, while the recent acceleration is due to dark energy, which behaves like a force.
  • There is a discussion about critical density and its implications for whether the universe will collapse into a Big Crunch, with some asserting that a universe at critical density would not collapse even without dark energy.
  • Some participants express concerns about the terminology used regarding dark energy, arguing that it should not be considered a separate force from gravity, but rather a different manifestation of gravitational effects depending on matter properties.
  • One participant highlights the importance of the relationship between matter density and pressure in determining the dynamics of expansion, noting that negative pressure is necessary for acceleration.

Areas of Agreement / Disagreement

Participants express multiple competing views on the nature of dark energy and its relationship with gravity, leading to an unresolved discussion regarding the implications for cosmic expansion and the potential for a Big Crunch.

Contextual Notes

Participants note that the understanding of dark energy and its effects on cosmic expansion is still developing, and there are unresolved questions about the definitions and implications of critical density.

TheIsland24
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In "A Brief History of Time" Hawking questions why the expansion of the universe is accelerating. I must be missing something. If the universe is expanding, its volume is constantly increasing. If its volume is increasing its density is decreasing, so there is more space between bodies/particles and less gravitational force. The farther these particles get from each other, the less resistance there will be on the expansion of the universe...therefore causing it to expand faster and faster. What would have to happen to cause a Big Crunch? Would the rate of the creation of new particles have to be greater than the rate at which the universe was expanding? Help me Out.
 
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TheIsland24 said:
In "A Brief History of Time" Hawking questions why the expansion of the universe is accelerating. I must be missing something. If the universe is expanding, its volume is constantly increasing. If its volume is increasing its density is decreasing, so there is more space between bodies/particles and less gravitational force. The farther these particles get from each other, the less resistance there will be on the expansion of the universe...therefore causing it to expand faster and faster. What would have to happen to cause a Big Crunch? Would the rate of the creation of new particles have to be greater than the rate at which the universe was expanding? Help me Out.

Expansion is not a force. It's just the movement of things apart from each other. If there was no gravity, then expansion would continue at the same rate... analogous to movement of particles at constant velocity.

With any gravity, expansion tends to slow down, because gravity pulls things together.

But, strangely, things appear to be moving aprt from each other faster, and faster... as if something is giving them an extra boost. The "something" is called "dark energy". And we don't really know anything more about it than it is whatever it is that gives that bit of an extra push to make thing increase in the speed at which they are dispersing.

The Big Crunch is an idea which applies if the force of gravity to pull things together is sufficiently strong to actually slow the expansion, or dispersion, and bring it to a stop, reverse it, and then start everything falling back together again. In terms of just two particles (rather than an entire universe of particles) it is analogous to the particles moving apart at less than escape velocity. They'll eventually stop, reverse, and start moving together. Same with a universe that has a "critical density" of mass and no dark energy.

Cheers -- sylas
 
TheIsland24 said:
I must be missing something.
You are.
TheIsland24 said:
If the universe is expanding, its volume is constantly increasing. If its volume is increasing its density is decreasing, so there is more space between bodies/particles and less gravitational force. The farther these particles get from each other, the less resistance there will be on the expansion of the universe...therefore causing it to expand faster and faster.
Gravity acts to slow the expansion, that is to say it decelerates it. The decrease in gravity due to the lower density means only that the rate of the acceleration of the expansion will decrease. In order for the acceleration to increase, a force must apparently be at work. We currently call that force "dark energy" but we are really only just beginning to understand it.
 
*shakes fist at fast-typing sylas*
 
There are two kinds of expansion:

1. The original expansion left over from the Big Bang (or inflation). This expansion acts like momentum, and is progressively slowed by the gravity of the mass-energy in the universe. This expansion does not act like a force. It cannot cause objects to separate unless the objects were already separating in the initial conditions.

2. The more recent acceleration of expansion over the last 7 Gy or so caused by Lambda, Dark Energy, the cosmological constant, whatever you want to call it. This expansion does act like a force. It can cause objects to begin separating even if they were not separating previously. And if they were already separating (e.g. in the Hubble flow) it will cause the rate of separation to increase.

Lambda is believed to impart sufficient acceleration to the expansion that the universe will never collapse in a Big Crunch. Instead, the expansion will continue accelerating until it asymptotically approaches the acceleration rate of Lambda alone, with the offsetting deceleration effect of gravity having become utterly insignificant, due to the ever-declining density of matter.

Keep in mind that even if there were no Lambda, the universe would not necessarily have collapsed in a Big Crunch. That depends on whether the matter density was sufficiently high compared to the expansion rate (Hubble rate). Such a universe would eventually collapse only if it were "overdense", meaning that it was above critical density. A universe exactly at critical density (and without any Lambda) would expand more and more slowly over time; the Hubble rate would asymptotically approach zero, but would never quite reach zero in finite time. The Hubble rate would never go negative, so such a universe would not collapse. This decreasing rate of deceleration is due to the decreasing effect of gravity, which in turn is due to the decreasing matter density, as you allude to in your OP. But adding Lambda to the mix changes the situation.
 
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Thank you Nutgeb! That explained it. So gravity cannot affect the resultant expansion of the big bang. So are you saying that gravity does affect Dark Energy?
 
TheIsland24 said:
Thank you Nutgeb! That explained it. So gravity cannot affect the resultant expansion of the big bang. So are you saying that gravity does affect Dark Energy?

Uh... nutgeb described near the end of his post the same effect of gravity on expansion that everyone else did. Gravitation attraction of matter retards, or slows, the rate of expansion.

He also described the critical density case, where which is a case where the density is not quite enough to to reverse the expansion back to contraction.
 
I think that talking about "dark energy" as if it's some force different from gravity is poor use of language.

General Relativity provides a connection between space-time and matter. If you fill the universe with different sorts of matter, the expansion behaves differently. Fill it with normal matter, and it decelerates. Fill it with radiation, and it decelerates even more rapidly. Fill it with one of many types of hypothetical matter now placed under the umbrella term "dark energy", though, and it accelerates. It's still the action of gravity that is affecting the expansion, not some new force. It's just that gravity acts differently depending upon the properties of the underlying matter.

The property in question that is important is the relationship between the density of the matter in question and its pressure. Radiation has positive pressure equal to one third of its energy density, and that positive pressure causes the expansion to slow more rapidly. Normal matter has no pressure (e.g. galaxies don't experience pressure between one another). To get acceleration, you have to have negative pressure that is more negative than minus one third the energy density. A cosmological constant, for instance, has negative pressure equal to the energy density.
 
Chalnoth said:
I think that talking about "dark energy" as if it's some force different from gravity is poor use of language.

General Relativity provides a connection between space-time and matter. If you fill the universe with different sorts of matter, the expansion behaves differently. Fill it with normal matter, and it decelerates. Fill it with radiation, and it decelerates even more rapidly. Fill it with one of many types of hypothetical matter now placed under the umbrella term "dark energy", though, and it accelerates. It's still the action of gravity that is affecting the expansion, not some new force. It's just that gravity acts differently depending upon the properties of the underlying matter.

Yes and no. The term "matter" is more limited than the term "energy". For example, radiation is not a "different form of matter", but you could call it a different form of energy. That's my one quibble here.

The key point is this. As the universe expands and disperses, the density of matter drops. The energy density of radiation (or matter at relativistic speeds, like neutrinos) drops even more quickly, because the cosmological redshift means energy density in a given co-moving region reduces by an additional factor on top of the number density of particles. And finally, the "dark energy" term, also called "cosmological constant", corresponds to an energy associated with the vacuum. The density of this energy remains fixed; it is like a property of empty space.

In general relativity, the crucial quantity is energy... whether it be in the form of matter, or radiation, or some energy associated with the vacuum. So there is indeed a strong sense in which dark energy is not an alternative to gravity at all. It's all still contained in the same relativistic account of gravity as the effects of matter.

What changes is the way energy density varies with the dispersal of expansion of the universe; this is what is different from matter, and from radiation.

Cheers -- sylas
 
  • #10
sylas said:
Yes and no. The term "matter" is more limited than the term "energy". For example, radiation is not a "different form of matter", but you could call it a different form of energy. That's my one quibble here.
I wouldn't agree with that. Photons are as much matter as electrons. It's just that we mean something specific when we talk about "normal" matter, which means non-relativistic fermions. Basically, I take issue with a definition of matter which excludes things like electrons and protons that are traveling too fast.

The problem with calling these things "energy" is that energy in itself is a property of matter. It isn't something that exists on its own.

sylas said:
And finally, the "dark energy" term, also called "cosmological constant", corresponds to an energy associated with the vacuum. The density of this energy remains fixed; it is like a property of empty space.
This isn't strictly accurate. The cosmological constant is one specific proposal for dark energy. There are others, though they all behave similarly at late times.

For example, so-called "quintessence" models of dark energy track the energy density of the most dominant form of matter at early times (meaning that early in the universe, this "quintessence" matter dilutes just like radiation, later like matter). At very late times, when the universe is sufficiently dilute, it starts to approach a constant energy density.
 
  • #11
What changes is the way energy density varies with the dispersal of expansion of the universe; this is what is different from matter, and from radiation.
If we call anything with \rho > 0 "matter", as Chalnoth obviously intended, all possible variations follow the same law, dE=-pdV:
\frac{d}{d t}\,(\rho\,a^3) = -p\,\frac{d}{d t}\,(a^3)
So I think it's ok to say that there may be all sorts matter or stuff or something with different equations of state, but all on an equal footing, as far as GR is concerned.
But I think we all agree anyway.
 
  • #12
Chalnoth said:
I wouldn't agree with that. Photons are as much matter as electrons.

Terminology... I think the standard definition of "matter" is stuff that has non-zero rest mass. This excludes photons. But it is a terminology point.

It's just that we mean something specific when we talk about "normal" matter, which means non-relativistic fermions. Basically, I take issue with a definition of matter which excludes things like electrons and protons that are traveling too fast.

I certainly don't exclude things on the basis of velocity. By my usage, which I think is pretty standard, the term matter excludes photons, but not relativistic protons or other particles with a non-zero rest mas. I noted explicitly that relativistic particles have an equation of state similar to photons.

The problem with calling these things "energy" is that energy in itself is a property of matter. It isn't something that exists on its own.

By normal usage, energy is a property of more than only matter... and dark energy is basically a property of the vacuum.

This isn't strictly accurate. The cosmological constant is one specific proposal for dark energy. There are others, though they all behave similarly at late times.

For example, so-called "quintessence" models of dark energy track the energy density of the most dominant form of matter at early times (meaning that early in the universe, this "quintessence" matter dilutes just like radiation, later like matter). At very late times, when the universe is sufficiently dilute, it starts to approach a constant energy density.

Granted. I was simplifying a bit... deliberately, I confess. But I think we are on the same page. I'm just clearing up how we use terms.

Cheers -- sylas
 
  • #13
If the universe has always existed --- is retrospectively infinite --- then there was no "big bang" that started it.

If we hypothesize that is true, then the expansion of the universe which we observe happening is not an expansion outward from a single point of initial explosion. There would have been no such beginning point. Another explanation of the expansion is needed.

Another type of expansion is the expansion that takes place with respect to a rising piece of bread dough.

Visualize a lump of rising dough that has raisins scattered throughout it. As the bread dough expands under the influence of the yeast --- aka dark energy --- the raisins move farther and farther apart from one another. The further any two raisins are located apart from one another in the matrix of the dough, the faster those two raisins will move apart from one another, and their rate of separation will steadily accelerate.

This seems analogous to what we are observing with our powerful telescopes. The farther things are away from us in space, the faster they are moving away from us (and us from them). It is as if the universe is structured very much like the raisinbread model. The "dough" is invisible and expanding "dark matter," and all of the corporeal structures imbedded within the dough --- planets, stars, people, what-have-you --- are the raisins.

The only two differences may be:

(1) that the corporeal "raisins" in the real universe --- what we call "matter" --- also expand at the same rate that the doughy dark matter expands, so that relative near spatial intervals appear to us to be unchanging; and

(2) that there is no limit --- outer edges --- of the universe, it being infinite in size as well as in age.

I expect that the latest expansion of the Hubble telescope's visual accuity has revealed more and more "raisins" out beyond our previous limits of observation. I expect that they are more and more red-shifted toward an ultimate point of invisibility where the separation rate between our planet and those distant bodies attains and exceeds the speed of light. Perhaps we are getting close to the point where we will be able to observe these distant bodies "wink out" of vivibility.
 
  • #14
LtDan said:
If the universe has always existed --- is retrospectively infinite --- then there was no "big bang" that started it.
The big bang theory, properly understood, does not include a beginning. It is generally recognized that the theory breaks down before you go that far back, and a different theory is needed to explain what happens at the earliest times. We don't yet know for certain how our region of the universe began, though the theoretical evidence indicates rather strongly that it had to begin at some point (though possibly from a pre-existing space-time).

LtDan said:
If we hypothesize that is true, then the expansion of the universe which we observe happening is not an expansion outward from a single point of initial explosion. There would have been no such beginning point. Another explanation of the expansion is needed.
That's not what the big bang theory says, though.

LtDan said:
Another type of expansion is the expansion that takes place with respect to a rising piece of bread dough.
This is a pretty good analogy for what the big bang theory actually says.

LtDan said:
(2) that there is no limit --- outer edges --- of the universe, it being infinite in size as well as in age.
Neither is necessarily the case. Our universe may be finite in size. It may be infinite. We don't know. Our region of the universe is almost certainly finite in age, but we don't know how old what it stemmed from is. That may be infinite in age. Or our region of the universe may have been what started it all off. We just don't know.

LtDan said:
I expect that the latest expansion of the Hubble telescope's visual accuity has revealed more and more "raisins" out beyond our previous limits of observation. I expect that they are more and more red-shifted toward an ultimate point of invisibility where the separation rate between our planet and those distant bodies attains and exceeds the speed of light. Perhaps we are getting close to the point where we will be able to observe these distant bodies "wink out" of vivibility.
Well, that won't happen. They'll just get gradually more and more redshifted. They only reach zero brightness as time goes to infinity. There's no point where you could say, "after this time, these objects are no longer visible."
 
  • #15
If the rate of separation between Earth and a visible far distant object in space eventually reaches and exceeds the speed of light, wouldn't that far distant object become invisible to us?
 
  • #16
LtDan said:
If the rate of separation between Earth and a visible far distant object in space eventually reaches and exceeds the speed of light, wouldn't that far distant object become invisible to us?
We can never see the photons that leave it after a certain time (not simply given by its recession velocity, but instead by the future expansion history of the universe). But this doesn't mean that we cease to see it: we see its after-image forever. It just gets dimmer and dimmer. And, as near as we can tell time slows and slows for this image as time goes forward, and the apparent age of the object in our after image asymptotically approaches the age at which the object crossed our horizon.

Note, however, that this is only true in an accelerating universe. If the universe were not accelerating, or stopped accelerating at some point in the future, then there would be no future horizon, and, given infinite time, we would be able to see the full history of all objects in the universe.
 
  • #17
There are two terms I do not understand: "future expansion history" and "asymptotically."
 
  • #18
LtDan said:
There are two terms I do not understand: "future expansion history" and "asymptotically."
future expansion history = the way the universe expands into the future.
asymptotically = behavior that a system approaches out to infinity.

Hopefully future expansion history is understandable. Asymptotically may take a little bit more work. A simple example would be this equation:

f(x) = 1/x.

In the above equation, f(x) approaches zero as x approaches infinity. This is known as asymptotic behavior: there isn't actually any number x for which f(x) = 0. But as x gets bigger and bigger, f(x) gets closer and closer to zero without actually hitting zero.
 
  • #19
Is it accurate to refer to our hypothetical infinite-aged and infinite-sized universe, operating in a "rising raisinbread" mode, as an "accelerating universe"?

Since our infinite universe has no outer edges, how can we judge the speed of the universe's expansion. One way would be by calculating expansion speed from the red shift observed in distant objects. Another would be by taking a chunk of the universe --- a chunk with observable edges to it --- and somehow measuring the speed at which that chunk of matter is expanding in size. Since all matter, both visible and invisible, is expanding in size at the same universal rate, it is impossible to measure any universal expansion growth against a constant measuring stick. The measuring stick is also expanding. The only way to discern and measure the expansion of our reference chunk is by referring to what we have been calling "gravity" since Newton's time.

The planet Earth is the handiest corporeal chunk of the universe to use in this exercise. It is expanding at a rate that causes objects located against it to stick to the planet's surface and to display the characteristic we call "weight."

Since the weight of such an object does not change from one second to the next, is it reasonable to assume that the outward movement of the Earth' surface is actually accelerating and not merely moving outward at a steady rate of speed? A steady rate of speed would seem to suffice to keep the planet in contact with its "companion," as long as the companion kept still. But if the companion were to, for instance, jump up in the air, there would seem to be nothing to prevent the companion from simply flying away. There would be no way for the planet's surface to catch up with the companion.

[In an old radio routine, Edgar Bergen was attempting to explain gravity to Mortimer Snerd. He asked Mortimer why, when he jumped up into the air, he returned to earth. Mortimeer replied, "I live there."]
 
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  • #20
LtDan said:
Is it accurate to refer to our hypothetical infinite-aged and infinite-sized universe, operating in a "rising raisinbread" mode, as an "accelerating universe"?
Yes, because the measured rate of expansion is accelerating.

LtDan said:
Since our infinite universe has no outer edges, how can we judge the speed of the universe's expansion. One way would be by calculating expansion speed from the red shift observed in distant objects. Another would be by taking a chunk of the universe --- a chunk with observable edges to it --- and somehow measuring the speed at which that chunk of matter is expanding in size. Since all matter, both visible and invisible, is expanding in size at the same universal rate, it is impossible to measure any universal expansion growth against a constant measuring stick. The measuring stick is also expanding. The only way to discern and measure the expansion of our reference chunk is by referring to what we have been calling "gravity" since Newton's time.
Well, no, the measurement of the rate of expansion is largely independent of the behavior of gravity.

LtDan said:
The planet Earth is the handiest corporeal chunk of the universe to use in this exercise. It is expanding at a rate that causes objects located against it to stick to the planet's surface and to display the characteristic we call "weight."
The Earth isn't expanding.

LtDan said:
Since the weight of such an object does not change from one second to the next, is it reasonable to assume that the outward movement of the Earth' surface is actually accelerating and not merely moving outward at a steady rate of speed? A steady rate of speed would seem to suffice to keep the planet in contact with its "companion," as long as the companion kept still. But if the companion were to, for instance, jump up in the air, there would seem to be nothing to prevent the companion from simply flying away. There would be no way for the planet's surface to catch up with the companion.
Ugh. You seem to be confusing the equivalence principle with actual acceleration. While a the existence of a uniform gravitational field is indistinguishable from acceleration, this does not mean that a gravitational field is acceleration. In particular, the gravitational field of a body like the Earth is not uniform at all, but changes from place to place (that is, it gets weaker as you move away from the Earth, and changes in direction as you go around the Earth). Because the gravitational field changes from place to place, there is no acceleration which can mimic the entire gravitational field. So the gravitational field of the Earth cannot be considered an acceleration.
 
  • #21
When you say "the Earth is not expanding," you forget that in our hypothetical raisinbread universe all matter expands.

Leaving hypothesis behind for a moment, I believe that the planet does, in many respects, behave as if it is expanding in size. Tectonic movements of the crustal plates, for instance, do not resemble the slight movements seen in the outer skin of a molten metal sphere suspended in a cooling liquid. In the molten sphere there is very little movement to be seen, but if the molten center of the sphere were to be steadily expanding in volume, fractures, spreading and subduction would take place as they take place with our planet's tectonic plates.
 
  • #22
LtDan said:
When you say "the Earth is not expanding," you forget that in our hypothetical raisinbread universe all matter expands.

No... he's TELLING you, correctly, that the expanding universe in cosmology, for which rising raisin bread is a simple analogy, does NOT have all matter expanding. Just like the raisins don't get larger as the break rises; galaxies, stars, and planets all remain the same size.

Cheers -- sylas
 
  • #23
Hi Sylas,


Whose raisinbread universe is it, anyway? If I make up a raisinbread hypothetical universe, I'm the one who gets to say whether or not the raisins rise just like the dough.

And I say they rise!

If the univrese is expanding --- and it sure does seem that it is --- then why shouldn't everything in the universe be expanding, including all "matter"?
 
  • #24
LtDan said:
Hi Sylas,


Whose raisinbread universe is it, anyway? If I make up a raisinbread hypothetical universe, I'm the one who gets to say whether or not the raisins rise just like the dough.

And I say they rise!

If the univrese is expanding --- and it sure does seem that it is --- then why shouldn't everything in the universe be expanding, including all "matter"?

Um... check the physicsforums rules, here; and in particular the section on speculative posts.

One of the main goals here is to discuss the current status of physics as practiced by the scientific community. In modern cosmology, the expansion of the universe is not a force driving things apart. One large scales galaxies are dispersing and separating from each other and they continue to do so by the "momentum" of their dispersal. Gravity works to pull them together, and apparently there is a "dark energy" that is pushing things apart; but on small spaces like a galaxy, or a solar system, gravity holds things together. They are gravitationally bound, and not flying apart at all.

If you have a DIFFERENT notion, all of you own, this may not be the best forum for you. Merely asserting things because you say so is not going to be permitted as a basis of discussion anywhere in the forum; though there are designated areas where you can propose some non-standard ideas as long as they are actually worked out with some regard to the realities of physics.

Cheers -- sylas
 
  • #25
Well the raisinbread universe theory is certainly speculative, although I think it makes a good bit of sense and isn't, therefore, "overly speculative."

Sylas, regarding "dark energy" driving galaxies apart from one another, do you think that the faint radio signal that seems to come from every direction might be the "sound" that the dark energy makes, and not the echo of a big bang?
 
  • #26
LtDan said:
Well the raisinbread universe theory is certainly speculative, although I think it makes a good bit of sense and isn't, therefore, "overly speculative."

The raisinbread is not a theory at all, but a mental picture than may help understand conventional cosmology. You've mixed up the actual physics with the simple similies used to try and help explain some of the concepts without going into the technical maths of the actual theory.

Sylas, regarding "dark energy" driving galaxies apart from one another, do you think that the faint radio signal that seems to come from every direction might be the "sound" that the dark energy makes, and not the echo of a big bang?

No, it definitely isn't.

Cheers -- sylas
 
  • #27
Sylas,

Do you have any notion about what that faint, pervasive radio signal is?

Cheers --- LtDan
 
  • #28
LtDan said:
Sylas,

Do you have any notion about what that faint, pervasive radio signal is?

Cheers --- LtDan

You appear to be speaking of the cosmic microwave background radiation, which is thermal radiation from early stages of the universe when it had cooled enough to form transparent neutral hydrogen., redshifted by a factor of about 1100.
 
  • #29
sylas said:
You appear to be speaking of the cosmic microwave background radiation, which is thermal radiation from early stages of the universe when it had cooled enough to form transparent neutral hydrogen., redshifted by a factor of about 1100.
Actually, I think he might be talking about this:
http://www.scienceagogo.com/news/20090008190614data_trunc_sys.shtml

We looked over this paper not too long ago, and I think the general conclusion is that it seems more likely this is a case of improper subtraction of the galactic signal than anything.
 
  • #30
That is an interesting article about the "new" radiation recently detected, but I was referring to the radiation detected by Penzias and Wilson that so many people believe --- and some say know --- is an echo of the Big Bang. I don't believe it is, but most others disagree. I think --- speculate --- that it's a humming sound or signal created by all matter as it expands in size.
 

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