Vighnesh Nagpal
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Why does dark energy increase along with the expansion of the universe ( I'm not even sure it does but if it dosen't please correct me 

wabbit said:this is the only form compatible with standard general relativity
Thanks for the correction, edited that - I guess I was using "standard" in an unduly restrictive sense here.PeterDonis said:Not really. It is the simplest form compatible with standard GR.
I think the way you worded this is slightly confusing.phinds said:It does and is well known to. It's not clear to me why it should, but the density of the "dark energy", whatever it is, remains constant as spacetime expands, so the total amount increases.
Excellent correction. Thanks. I was going to add, and clearly should have, that the implication of (or really just another way of saying) "density of dark energy remains constant" is that it does not dilute within a given cosmologically large volume but the matter density does dilute.Chalnoth said:I think the way you worded this is slightly confusing.
The density of dark energy remains constant, but everything else dilutes with the expansion. So over time, the dark energy makes up a larger fraction of the energy density. It doesn't increase: everything else just decreases.
To qualify this somewhat, the following paper (not completely sure if this is an acceptable source - will remove if not) assesses current observational constraints on dark energy anisotropy and inhomogeneity (and hints of a possible large scale dipole moment in dark energy) : Leandros Perivolaropoulos : Large Scale Cosmological Anomalies and Inhomogeneous Dark Energywabbit said:there is so far no observational evidence that forces cosmologists to abandon this assumption and go for something more general
A wide range of large scale observations hint towards possible modifications on the standard cosmological model which is based on a homogeneous and isotropic universe with a small cosmological constant and matter. These observations, also known as "cosmic anomalies" include unexpected Cosmic Microwave Background perturbations on large angular scales, large dipolar peculiar velocity flows of galaxies ("bulk flows"), the measurement of inhomogenous values of the fine structure constant on cosmological scales ("alpha dipole") and other effects. The presence of the observational anomalies could either be a large statistical fluctuation in the context of {\lcdm} or it could indicate a non-trivial departure from the cosmological principle on Hubble scales. Such a departure is very much constrained by cosmological observations for matter. For dark energy however there are no significant observational constraints for Hubble scale inhomogeneities. In this brief review I discuss some of the theoretical models that can naturally lead to inhomogeneous dark energy, their observational constraints and their potential to explain the large scale cosmic anomalies.
Vighnesh Nagpal said:Why does dark energy increase along with the expansion of the universe ( I'm not even sure it does but if it dosen't please correct me
Excellent reference. I really like Carroll; I think he's a good explainer. I have a "Teaching Company" set of 12 half-hour video lectures by him on "Dark Matter; Dark Energy" and they're excellent.stevebd1 said:I always thought this was a good overview of dark energy and the expanding universe-
http://preposterousuniverse.com/writings/skytel-mar05.pdf
Vighnesh, I don't know of any scientific reason to think that "dark energy" actually arises from any form of energy. Some people think of it that way and others don't. All we observe is a small residual expansion rate that corresponds to a curvature constant that appears naturally on the lefthand side of the GR equation. In my experience it confuses people to think of it as some kind of energy---it's just a slight built-in spacetime curvature.Vighnesh Nagpal said:Why does dark energy increase along with the expansion of the universe ( I'm not even sure it does but if it dosen't please correct me![]()
marcus said:This fractional distance growth rate was much larger in the early universe and has been steadily declining ever since. It is expected to continue declining but not to reach zero. Instead it is expected to level off at 1.83 x 10-18 per second.
Think about this: You are going 100mph and you are accelerating at 20mph per hr, so in an hour you will be going 120 mph. At that point, your acceleration decreases to 19mph per hr, so in one more hour you will be going 139mph. Does that seem to you like "slowing down"?Phynos said:If the expansion is accelerating, why is this fractional distance growth rate decreasing? Doesn't that imply the acceleration is actually negative and that things are slowing down? Or am I misunderstanding what you're saying?
Phynos said:If the expansion is accelerating, why is this fractional distance growth rate decreasing? Doesn't that imply the acceleration is actually negative and that things are slowing down? Or am I misunderstanding what you're saying?
phinds said:Think about this: You are going 100mph and you are accelerating at 20mph per hr, so in an hour you will be going 120 mph. At that point, your acceleration decreases to 19mph per hr, so in one more hour you will be going 139mph. Does that seem to you like "slowing down"?
marcus said:that is a verbal problem, Phyrnos. the word "accelerating" is confusing people. the expansion rate has always been decreasing since the very early universe and according to the standard cosmic model (called LambdaColdDarkMatter, or LCDM) we expect it to continue decreasing, just not to get down to zero but to kind of level out at a longterm rate.
The big discovery in 1998 was that the longterm rate is not zero but is actually a small positive rate.
marcus said:I don't like the word "acceleration" in this context because for most of us it has mental associations with driving a car. Driving a car is not a good metaphor for the pattern of cosmic distance growth described by Hubble Law. The analogies are weak, and awkward, and lead to confusion. A better analogy would be money in a savings account at the bank where the interest rate is gradually declining. If the fractional growth rate is declining GRADUALLY ENOUGH then the account can still grow each year by a larger dollar amount (because the principal is increasing). AFAICS the minute you use the word "acceleration" and start thinking about driving a car you have lost touch with the actual process occurring in nature.
Perfect! That's probably how I should have started off.wabbit said:And following this I checked other definitions for a few expressions we hear, hope I got this right:
Hubble scale = scale factor = a(t) or R(t), the characteristic scale of the universe, its size if finite.
Hubble parameter = Hubble rate = H(t) =## \dot a(t)\over a(t)##, the logarithmic growth rate of that scale.
Hubble constant = current value of the Hubble rate
Just need to be careful...
BillyT said:Is it true that:
(3) Is conservation of energy law, ... false on scale of the universe?
marcus said:...everybody just becomes farther apart.
It isn't governed by laws of KE that you are used to and that you invoke. It doesn't take energy to accelerate it. It is dynamic changing geometry, not ordinary motion. It is normal for the growth of distances to be faster than c. The distances to MOST of the galaxies that we can see with a telescope are increasing faster than c. The great majority are.
So the pattern of distance growth (expressed in Hubble Law) should not be thought of as ordinary familiar motion thru space that we are used to. It does not obey the same rules. Just some friendly advice---of course you can think of geometric expansion as motion thru space if you like, but it seems to work out better not to.
Think about it this way: each location is the same, a comoving object sees a uniform matter distribution around it : what would it mean for it to "resist the expansion" ? In which direction would it "slip" if it were to do so?why don't the comoving masses resist and slip against the expansion
That's an interesting way to express it, as a pressure - which we can compare to the standard atmospheric pressure of ~100 kilopascals.marcus said:So the present energy density of the universe (radiation, ordinary matter and dark matter mass energy equiv) is 0.24 nanopascal.
Thanks. I understand that the amount of KE depends upon what frame is taken to be at rest; so in Earth's frame, the Earth's translational KE is zero; However, Is it not true that given any choice of a "rest frame," the objects not at rest in it have KE that is increasing with time? (as is their mutual attraction PE). I also know there is no preferred rest point - no "center of the universe" but am in doubt whether or not their is a "mass center" of the universe. - The grand "Barycenter." but doubt it is stationary point in space.marcus said:BillyT, you run a risk of confusing your listeners or yourself if you think of the pattern of growing distances as if it were ordinary motion like what we are familiar with. Nobody GETS anywhere by it. ...
I thought the increase of KE, wrt any point chosen to be "at rest" was due to the work done on the objects with increasing KE (and mutual PE). Is this POV wrong?marcus said:It doesn't take energy to accelerate it. It is dynamic changing geometry, not ordinary motion.
I think it is simply not applicable in this context. The comoving objects are at rest with respect to each other, they are not moving at all (even though their distance is increasing ! ) and have no kinetic energy associated to this increasing distance.BillyT said:I thought the increase of KE, wrt any point chosen to be "at rest" was due to the work done on the objects with increasing KE (and mutual PE). Is this POV wrong?
Yes, but:wabbit said:@bahamagreen ... I think the "balloon analogy" ... helps in understanding this. ...
I think so. It sounds to me like you are confusing recession (the growth of distance between widely separated objects) with ordinary motion.BillyT said:... Is this POV wrong?
Is this POV, sort of by redefining KE, an effort to save "conservation of energy"?wabbit said:I think it is simply not applicable in this context. The comoving objects are at rest with respect to each other, they are not moving at all (even though their distance is increasing ! ) and have no kinetic energy associated to this increasing distance.
http://www.phinds.com/balloonanalogy/
Edit "not moving" may or may not be an accepted way to state it, but I think this is a matter of semantics - maybe I should have said "not moving in the way that we usually think of moving". Or just, "no kinetic energy". But this doesn't change the point.
Not at all I think. First conservation energy is not saved in GR, so that would be a failed attempt. But the point is "what is the velocity that goes into KE?". And it is not the recession velocity of comoving objects.Is this POV, sort of by redefining KE, and effort to save "conservation of energy"?
I would say this at least sounds like a perfectly reasonable interpretation of the equations - then again, you say Einstein said it first, so I feel quite safe hereQuds Akbar said:Einstein once suggested that it might as well be another property of space itself. So I think that as space expands there is more dark energy. Though dark energy may not even exist at all, but most observations suggest it does exist. So it could be just a property of space itself.
BillyT said:Yes, but:
If gas is flowing into the balloon at constant rate, ...
wabbit said:@bahamagreen : The comoving objects discussed are indeed inertial, and their proper acceleration is zero - it is only as you say their comoving distance that is changing (and accelerating), but this is not due to proper movement, only to the expansion of space.
Think about it this way: each location is the same, a comoving object sees a uniform matter distribution around it : what would it mean for it to "resist the expansion" ? In which direction would it "slip" if it were to do so?
I think the "balloon analogy" (see the excellent explanation linked to in phind's signature) helps in understanding this.
Disclaimer: not a physicist here, just echoing what others have said.