Nature of the cosmological constant

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Discussion Overview

The discussion revolves around the nature of the cosmological constant (\(\Lambda\)) within the context of the Hilbert action and its implications for the Einstein equations. Participants explore its interpretation as either a geometrical parameter or as related to matter fields, examining the theoretical underpinnings and potential contributions from quantum fields.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant questions why the term \(\Lambda g_{\mu \nu}\) is considered related to matter fields when the action does not include them, suggesting it should represent an energy of 'pure' space-time.
  • Another participant interprets \(\Lambda\) as a geometrical parameter, hinting at a connection to concepts like the antimatter "sea" from Dirac's formulation of quantum mechanics.
  • It is proposed that the cosmological constant may be fundamental to gravity or induced by a field with a specific stress-energy, reflecting differing interpretations of its role.
  • One participant expresses skepticism about the necessity of the cosmological constant as a law of nature, suggesting that while it may be an interesting problem, it is overrated.
  • A later reply discusses the possibility of deriving an effective cosmological constant from the contributions of bosonic and fermionic fields, although details on quantum field theory (QFT) are not provided.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the interpretation of the cosmological constant, with multiple competing views presented regarding its nature and implications.

Contextual Notes

There are unresolved questions regarding the relationship between the cosmological constant and matter fields, as well as the implications of quantum field contributions. The discussion reflects a range of interpretations without definitive conclusions.

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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Sorry, but my intention was to post this in the Special & General Relativity forum. Is it possible to shift the thread? Thanks.
 
no problem...
 
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.
 
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.
 
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.
 
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.
 

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