Cosmological Constant Term in Einstein Equations

Sometimes the factor of 1/2 is included in Lambda, and sometimes it is not. It is a matter of convention and does not change the physical content of the equations. In summary, the Einstein Equations with a cosmological constant include a term with a plus sign and without a factor of 1/2 in front of it, which is a matter of convention and does not affect the physical content of the equations.
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kent davidge
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One side of the Einstein Equations with a cosmological constant is ##R_{\mu \nu} - (1/2) Rg_{\mu \nu} + \Lambda g_{\mu \nu}##.

Question is, why the cosmological constant term appears with a plus sign and without a factor of 1/2 in front of it?

I guess it may be because ##\Lambda## is (in principle) just any constant, so both the minus sign and the 1/2 factor can be absorbed into it?
 
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  • #2
kent davidge said:
Question is, why the cosmological constant term appears with a plus sign and without a factor of 1/2 in front of it?

The sign is just a convention, since ##\Lambda## can have either sign.

Why would you expect a factor of 1/2 in front?
 
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It depends on how you write down Lambda in the action.
 
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1. What is the cosmological constant term in Einstein's equations?

The cosmological constant term, denoted as Λ (lambda), is a constant value that was added to Einstein's equations of general relativity to account for the observed expansion of the universe. It represents the energy density of the vacuum of space and is responsible for the accelerated expansion of the universe.

2. How does the cosmological constant affect the universe?

The cosmological constant has a major impact on the universe as it determines the overall curvature of space-time and the rate of expansion of the universe. A positive value of Λ leads to a flat or positively curved universe, while a negative value would result in a negatively curved universe. It also affects the rate of expansion, with a larger Λ leading to a faster expansion.

3. Why did Einstein introduce the cosmological constant?

Einstein initially introduced the cosmological constant in his equations to counteract the effects of gravity and maintain a static universe. However, after the discovery of the expanding universe by Edwin Hubble, Einstein abandoned the constant, calling it his "biggest blunder". It was later reintroduced by other scientists to explain the observed acceleration of the universe.

4. How is the value of the cosmological constant determined?

The value of the cosmological constant is still a topic of debate and research in the scientific community. Currently, it is estimated to be a very small number, around 10^-29 g/cm^3. This value is determined through observations of the expansion rate of the universe and the cosmic microwave background radiation, as well as theoretical calculations and simulations.

5. Can the cosmological constant change over time?

According to the current understanding of the cosmological constant, it is considered to be a constant value that does not change over time. However, some theories suggest that it may vary over long periods of time or in different regions of the universe. This is still a topic of ongoing research and debate in the scientific community.

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