Nature of the cosmological constant

In summary, the Einstein equations can be obtained by adding a scalar to the Hilbert action and taking the energy of space-time to be proportional to the metric. The cosmological constant, represented by \Lambda, can be interpreted as a geometrical parameter or induced by a field with stress-energy. The relationship between the cosmological constant and matter fields is still a matter of interpretation and has not been definitively proven.
  • #1
hellfire
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If one adds a scalar to the Hilbert action without considering any matter fields,

[tex] S = \int {d^nx {\sqrt -g} (R - 2 \Lambda) [/tex]

one gets the Einstein equations as:

[tex] R_{\mu \nu} - \frac{1}{2} R g_{\mu \nu} + \Lambda g_{\mu \nu} = 0 [/tex]

Now, one can take

[tex] T_{\mu \nu} = - \frac{\Lambda}{8 \pi G} g_{\mu \nu} [/tex]

as an energy of space-time, and get

[tex] G_{\mu \nu} = 8 \pi G T_{\mu \nu} [/tex]

I have read several times that this energy is considered to be the energy density of empty space. Calculations are then made considering contributions of the ground state of quantum fields (bosons and fermions) leading to different values depending on different assumptions for this calculation.

What I do not understand is why [tex]\inline \Lambda g_{\mu \nu} [/tex] is considered to be related to matter fields, since the defined action above did not include them (did it?). Shouldn’t this term be an energy of, let's say, ‘pure’ space-time?
 
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  • #2
Sorry, but my intention was to post this in the Special & General Relativity forum. Is it possible to shift the thread? Thanks.
 
  • #3
no problem...
 
  • #4
I have always seen [tex]\Lambda[/tex] interpretted as a geometrical (as opposed to material) parameter. My only vague idea would be that it might have something to do with the antimatter "sea" that I have heard about regarding Dirac's formulation of QM.
 
  • #5
You're right that it doesn't necessarily have anything to do with matter. Its just interpretation right now. You can take the point of view that the constant is fundamental to gravity, or that it is induced in cosmological situations by a field with the stress energy you wrote down.

In other words, your action might represent just gravity or gravity+other field. Is it ever possible to have an experimental situation with lambda=0? There is no evidence one way or the other.

Given that, many people still think that just accepting the constant as a law of nature is inelegant, so they try to explain it (and have failed spectacularly).

My personal opinion is that it is an overrated problem. There might be something interesting there, but I'm not convinced that there has to be.
 
  • #6
Stingray said:
You're right that it doesn't necessarily have anything to do with matter. Its just interpretation right now.
I see, this seams reasonable, but in light of this interpretation, shall I assume that adding up the contribution of bosonic and fermionic fields should lead to the net effect of a scalar field? How can this be proved?

Regards.
 
  • #7
hellfire said:
I see, this seams reasonable, but in light of this interpretation, shall I assume that adding up the contribution of bosonic and fermionic fields should lead to the net effect of a scalar field? How can this be proved?

I don't know the details on the QFT side, but given a Lagrangian, you can compute a stress-energy tensor. If that's proportional to the metric, then it acts like an effective cosmological constant.
 

FAQ: Nature of the cosmological constant

What is the nature of the cosmological constant?

The cosmological constant was first introduced by Albert Einstein in his theory of general relativity as a way to account for the observed expansion of the universe. It is a term in the equations of general relativity that represents the energy density of empty space.

How does the cosmological constant affect the expansion of the universe?

The cosmological constant has a repulsive effect on the expansion of the universe, causing it to accelerate rather than slow down. This is because the energy density of empty space remains constant as the universe expands, leading to a greater overall energy density and therefore a greater expansion rate.

Is the cosmological constant constant?

The name "cosmological constant" can be misleading, as it is not actually a constant in the traditional sense. It is a variable that can take on different values depending on the energy density of the universe. In the early universe, the cosmological constant was likely much larger than it is today, leading to a rapid expansion known as inflation.

What evidence supports the existence of the cosmological constant?

The existence of the cosmological constant is supported by several lines of evidence, including observations of the accelerated expansion of the universe, the cosmic microwave background radiation, and the distribution of galaxies. These observations are consistent with the predictions of theories that include a cosmological constant.

What are some current theories about the nature of the cosmological constant?

There are several theories that attempt to explain the nature of the cosmological constant, including the "vacuum energy" theory which suggests that empty space contains a non-zero energy density, and the "quintessence" theory which proposes a dynamic scalar field that drives the expansion of the universe. However, the true nature of the cosmological constant is still not fully understood and remains a subject of ongoing research and debate among scientists.

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