Graduate Couldn't the cosmological constant also have some sort of "dynamics"?

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The discussion centers on the nature of the cosmological constant, questioning whether it should be treated as a true constant or a variable influenced by spacetime dynamics. The simplest model, which assumes it is a constant, is favored due to a lack of evidence supporting its variability. While it is possible to construct models where the cosmological constant changes over time, these often yield results equivalent to a constant when compared with current data. The use of scalar fields in advanced general relativity textbooks illustrates this point, but ultimately, the additional complexity does not enhance predictive power with existing observations. Thus, the cosmological constant remains treated as a constant in cosmological models.
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Why should we believe that the cosmological constant is indeed a constant, and not another parameter that changes with spacetime dynamics?

Obviously it would make the calculations even more intractable; but who said that life in the universe is easy?!
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:oldeek:
 
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mad mathematician said:
Why should we believe that the cosmological constant is indeed a constant, and not another parameter that changes with spacetime dynamics?
Because a constant is the simplest model, and we have no evidence that it's not constant, so we use the simplest model that's consistent with the evidence.
 
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PeterDonis said:
Because a constant is the simplest model, and we have no evidence that it's not constant, so we use the simplest model that's consistent with the evidence.
I wonder how difficult it would be to to write down a model where it changes with time.
 
mad mathematician said:
I wonder how difficult it would be to to write down a model where it changes with time.
We usually call it "dark energy" when it's not assumed to be perfectly constant.
 
mad mathematician said:
I wonder how difficult it would be to to write down a model where it changes with time.
It's straightforward to write down the model; indeed doing that is an exercise in some advanced GR textbooks. The usual way is to use a scalar field.

But when you compare the model with data, you find that the field never changes, so it ends up being equivalent to a cosmological constant that is constant. Which means all the extra work you put into your model got you nothing in terms of predictive power. At least, not with the data we have now.
 
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