A question on the meaning of dark energy

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Discussion Overview

The discussion revolves around the nature of dark energy, questioning whether it can be considered "energy" in the traditional sense and exploring its implications for the expansion of the Universe. Participants examine various theoretical frameworks, including the cosmological constant and quintessence, while also addressing the concept of work in the context of General Relativity.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants question if dark energy is truly energy and whether work is being done in the expansion of the Universe, suggesting that significant work would be required to move galaxies apart against gravitational forces.
  • Others assert that dark energy contributes to the vacuum energy-density and is linked to the cosmological constant, with its effects described by negative pressure relations.
  • A participant mentions that the cosmological constant is a simpler explanation for dark energy compared to quintessence, which is viewed as a more complex model.
  • Concerns are raised about the applicability of the concept of work in General Relativity, with some arguing that in an expanding universe, energy conservation becomes problematic.
  • Some participants propose that dark energy might be an illusion, referencing various papers that critique or support this idea.
  • There is a discussion about the implications of structure formation on the expansion rate of the Universe, suggesting that voids may expand faster than overdense regions.
  • One participant introduces the term "smooth tension" as a potentially better descriptor for dark energy, emphasizing its uniformity and negative pressure.

Areas of Agreement / Disagreement

Participants express a range of views on the nature of dark energy, with no consensus reached. While some support the cosmological constant as the leading explanation, others advocate for alternative models like quintessence or the idea that dark energy is an illusion. The discussion remains unresolved regarding the implications of these theories and their observational support.

Contextual Notes

Participants note that the application of traditional concepts like work and energy conservation in an expanding universe is complex and may not align with classical interpretations. The discussion also highlights the evolving nature of research in this area, with references to various papers that present differing perspectives on dark energy.

Who May Find This Useful

This discussion may be of interest to those studying cosmology, theoretical physics, or anyone curious about the current debates surrounding dark energy and its implications for the Universe's expansion.

Tanelorn
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I have wondered about this for some time:

Is dark energy really energy and is work actually being done when it causes the Universe to expand?

It seems to me that work is being done in moving all the Galaxies further apart than they were, over coming their gravitational pull. For example a lot of work would need to be done to move the Earth into an orbit further from the sun.

So what is the source of this energy? If it is some kind of stored potential energy then what is its form and where is it stored?

I vaguely recall someone saying that the word energy is not a very good word for describing the effect.
 
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No one knows what dark energy really is or understands the mechanism behind it. However we do know how it influences expansion. In the sense that it contributes to the vacuum energy-density. Keep in mind dark energy is merely one possibility of the cosmological constant. The work is done by its negative pressure relations. Whose energy-density to pressure relation is determined by its equation of state. http://en.wikipedia.org/wiki/Equation_of_state_(cosmology)
 
yeah I did get that backwards, What is the status of quintessence now, last I heard its disfavored?
 
Sadly, this is beyond my area of expertise. As far as I know though, all the observations are consistent with the cosmological constant. Since the cosmological constant is simpler (it's a constant of integration and not a dynamical process) perhaps applying Occam's Razor means we should favor it over more complicated models like Quintessence. However, since Quintessence predicts a dynamical acceleration, this should be, at least in principle, observable. Whether our current technology can observe these dynamics, I cannot say. So, probably, we have to wait for better data to rule out one or the other.
 
Tanelorn said:
I have wondered about this for some time:

Is dark energy really energy and is work actually being done when it causes the Universe to expand?
Work isn't a term that is used very often within General Relativity, and I'm not sure it can be applied in general.

But in a homogeneous, isotropic expanding universe, it works:
If you consider a hypothetical box around a co-moving volume of space, and consider the work exerted on the walls of that box by the stuff inside it, you get an answer which precisely coincides with the change in energy within that co-moving volume.

For example, consider a universe with nothing but a cosmological constant at some density ##\rho_\Lambda##. Now expand that volume from ##a \rightarrow a + da## along each side . The volume increase is ##3a^2da##, while the "work" on each of the six sides is ##-\rho_\Lambda \cdot 1/2 a^2 da##, since ##p_\Lambda = -\rho_\Lambda## (ignoring terms with ##da^2## in each case).

So the increase in energy is ##3\rho_\Lambda a^2 da##, while the work done is ##-3\rho_\Lambda a^2 da##. You can imagine the dark energy as performing negative work, and gaining energy as a result.
 
The Law of the Conservation of Energy is problematical in an expanding Universe. Not only is the potential energy between two objects (separated by cosmological distances) reduced as the distance between them increases, but speeds and frequencies also diminish ('lose' energy) for particles or waves traveling during such expansion. If Energy is conserved (Energy/Mass/Momentum/Stress(Pressure)) then it has to GO somewhere, meaning that dark energy must be that.
 
abitslow said:
The Law of the Conservation of Energy is problematical in an expanding Universe. Not only is the potential energy between two objects (separated by cosmological distances) reduced as the distance between them increases, but speeds and frequencies also diminish ('lose' energy) for particles or waves traveling during such expansion. If Energy is conserved (Energy/Mass/Momentum/Stress(Pressure)) then it has to GO somewhere, meaning that dark energy must be that.

An expanding universe like the FRW metric has no time-like Killing vectors, only space-like ones. Therefore particle motion in an expanding universe does not conserve energy (material particles slow down, radiation gets red shifted). The "potential energy" of the gravitational field is a very touchy subject in General Relativity since the gravitational field is no longer a force, but a curvature in space-time.
 
It is a possibility [albeit, not wildly popular] that dark energy is an illusion - e.g., http://arxiv.org/abs/0712.0370, Local Void vs Dark Energy: Confrontation with WMAP and Type Ia Supernovae.
 
  • #10
  • #13
From 05:45 in this clip, dark energy is masterfully -and relatively simply- defined. A far better name is in fact "smooth tension":



Smooth because it is uniform throughout the whole universe.

Tension because is has negative pressure, ie it rends things apart, separating objects from each other.

Today we only know of positive pressure, eg that of particles impacting against the wall of a vessel. The energy/momentum of these particles are positive metrics. With dark enery, one is talking about negative values for these metrics.IH
 
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  • #14
Chronos said:
It is a possibility [albeit, not wildly popular] that dark energy is an illusion - e.g., http://arxiv.org/abs/0712.0370, Local Void vs Dark Energy: Confrontation with WMAP and Type Ia Supernovae.

It has been my understanding that the void models are increasingly difficult to reconcile with data. The most recent paper you've cited is over two years old. It would be nice to see what the latest data have to say. I haven't been following this area myself.

Perhaps it's worth noting that there is also another alternative to dark energy that has been proposed, namely the backeaction of structure formation on the expansion rate. My understanding is that the basic idea is that voids expand faster than overdense regions and as they do their relative fraction of the volume of the universe grows, thus increasing the average expansion rate. I think it's more of an idea at this point and it's not clear whether it can be a viable alternative. Here's a recent review:

http://arxiv.org/abs/1112.5335
 
  • #15
Chalnoth said:
Work isn't a term that is used very often within General Relativity, and I'm not sure it can be applied in general.

But in a homogeneous, isotropic expanding universe, it works:
If you consider a hypothetical box around a co-moving volume of space, and consider the work exerted on the walls of that box by the stuff inside it, you get an answer which precisely coincides with the change in energy within that co-moving volume.

For example, consider a universe with nothing but a cosmological constant at some density ##\rho_\Lambda##. Now expand that volume from ##a \rightarrow a + da## along each side . The volume increase is ##3a^2da##, while the "work" on each of the six sides is ##-\rho_\Lambda \cdot 1/2 a^2 da##, since ##p_\Lambda = -\rho_\Lambda## (ignoring terms with ##da^2## in each case).

So the increase in energy is ##3\rho_\Lambda a^2 da##, while the work done is ##-3\rho_\Lambda a^2 da##. You can imagine the dark energy as performing negative work, and gaining energy as a result.


Chalnoth, is this interpretation not like the pressure of gas atoms on a container wall? If so would this approach apply to the case of a box full of galaxies?
 
  • #16
Tanelorn said:
Chalnoth, is this interpretation not like the pressure of gas atoms on a container wall? If so would this approach apply to the case of a box full of galaxies?
I think a better way to think of it is in terms of a volume of hot gas expanding into a vacuum. If I recall, you can use the same sort of argument to get the correct cooling rate of the expanding gas.
 
  • #17
Galaxies don't interact with each other like gas atoms do. Gravitational attraction is small between gas atoms and Galaxies which collide do not bounce off each other, instead they merge. So there is no net force causing them to expand unless we add in the dark energy expansion of space idea.
 

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