Non-Constant Cosmo-Constant: Controversy in GR?

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SUMMARY

The discussion centers on the introduction of a variable Cosmological Constant within the framework of General Relativity (GR) through the Hilbert action. It highlights the possibility of deriving varying cosmological constants from Kaluza-Klein reductions of higher-dimensional theories or by manually incorporating them into the model. The approach involves adding scalar fields to the Lagrangian, which, when combined with a suitable potential term, can lead to the dynamic generation of a non-zero cosmological constant. This method emphasizes the flexibility of scalar fields in modifying gravitational theories.

PREREQUISITES
  • Understanding of General Relativity and the Hilbert action
  • Familiarity with Kaluza-Klein theory and dimensional reduction
  • Knowledge of scalar fields and their role in Lagrangian mechanics
  • Basic concepts of potential terms in field theory
NEXT STEPS
  • Research the implications of variable Cosmological Constants in modern cosmology
  • Study Kaluza-Klein theory and its applications in higher-dimensional physics
  • Explore the role of scalar fields in Lagrangian formulations
  • Investigate the dynamics of potential terms in field theories
USEFUL FOR

The discussion is beneficial for theoretical physicists, cosmologists, and researchers interested in advanced concepts of General Relativity and modifications to gravitational theories.

ChrisVer
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I think that in the Hilbert action for the General Relativity /gravity, one can add a constant scalar quantity, which we call the Cosmological Constant.
I am wondering though, how can someone suggest ( after introducing it as a constant ) that this quantity could in fact vary?
 
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I see varying cosmological constants all the time. This comes straightforwardly out of Kaluza-Klein reductions from higher-dimensional theories, or you can just put it in by hand.

This is something you typically do if you want the cosmological constant to be an emergent phenomenon, as follows:

Put some scalar fields in your Lagrangian with the usual kinetic term (or you can put in a sigma model kinetic term with some target space), and also throw in a potential term. For the right choice of potential, your scalars will want to asymptotically approach nonzero constants, thus dynamically generating your cosmological constant.

Scalars are very flexible and can turn up anywhere in the Lagrangian, including as coupling constants for gauge fields.
 

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