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 and its potential variability in relation to spacetime dynamics. Participants argue that the cosmological constant is treated as a constant due to the lack of evidence supporting its variability, making it the simplest model consistent with current data. The concept of "dark energy" is introduced as a framework for models that allow for changes over time, but these models often revert to a constant when compared with observational data. Ultimately, the consensus is that while dynamic models can be constructed, they do not provide additional predictive power based on existing evidence.

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  • Basic knowledge of General Relativity (GR)
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mad mathematician
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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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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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