Meaning of cosmological constant ?

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SUMMARY

The cosmological constant, denoted as Lambda (Λ), has dimensions of 1/L² in the geometrized unit system of general relativity, representing energy density. Contrary to the misconception that its value evolves as 1/R², it remains constant over time. For a deeper understanding of its implications, particularly regarding characteristic distances, one should refer to section 7 of Padmanabhan's "Cosmological Constant - the Weight of the Vacuum." This discussion clarifies the relationship between the cosmological constant and the stress-energy tensor in spacetime models.

PREREQUISITES
  • Understanding of general relativity and its geometrized unit system
  • Familiarity with the concepts of energy density and curvature in cosmology
  • Knowledge of the stress-energy tensor and its components
  • Basic grasp of cosmological models and the evolution of the universe
NEXT STEPS
  • Read section 7 of Padmanabhan's "Cosmological Constant - the Weight of the Vacuum"
  • Explore the implications of the cosmological constant on the universe's expansion
  • Investigate the relationship between curvature and energy density in cosmological models
  • Study the role of the stress-energy tensor in general relativity
USEFUL FOR

Astronomers, physicists, and cosmologists interested in the implications of the cosmological constant on the universe's evolution and structure.

notknowing
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Incredibly much has been written about the cosmological constant and all its implications on the evolution of the universe. I want to ask however a more basic question about it. The cosmological constant has the dimension of 1/R^2. So supposing this constant is non-zero, its value points to the existence of some characteristic distance or radius. The Schwarzschild radius for instance has a clear understandable meaning but what could be the meaning of the radius associated with the cosmological constant? The only thing which comes to (my) mind is the radius of the universe itself. What other opinions exist (or are described in literature - related to "radius")?


Rudi Van Nieuwenhove
 
Space news on Phys.org
The cosmological constant has a value whose units are energy. I'm not sure what you mean by saying 'it has the dimensions of 1/R^2"?

If you mean that the energy density of the cosmological constant evolves as 1/R^2 where R is the scale factor that is incorrect. Curvature evolves in that way (in the way it is represented in cosmology) but the cosmological constant, unsurprisingly, remains constant for all time.
 
The dimensions of 1/L2 for the cosmological constant are correct in the usual geometrized unit system of general relativity. To find a deeper meaning to such a length scale one should go beyond general relativity, see for example section 7 of Padmanabhan's Cosmological Constant - the Weight of the Vacuum.
 
It might help to point out that in geometric units, energy density (and sectional curvatures, e.g. the components of the Riemann curvature tensor) have the units of reciprocal area. Since Lambda contributes a diagonal term to the stress-energy tensor of our spacetime models, with the entries proportional to Lambda (in any frame!), this represents an energy density and has the units of reciprocal area.
 
hellfire said:
The dimensions of 1/L2 for the cosmological constant are correct in the usual geometrized unit system of general relativity. To find a deeper meaning to such a length scale one should go beyond general relativity, see for example section 7 of Padmanabhan's Cosmological Constant - the Weight of the Vacuum.


Thanks for this interesting reference. This means a lot of reading (114 pages)!
 

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