Using Einstein field equation

In summary, the equation Gµv + Λgµv = (8πG/c4)Tµv involves tensor indices mu and nu, representing two-tensors, and matrices G, g, and T. The cosmological constant, originally dismissed, has regained interest due to its ability to explain certain observations in the universe, such as the acceleration of expansion and unexpected energy content. Further understanding of these concepts is recommended before delving into more advanced questions.
  • #1
kashiark
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Gµv + Λgµv = (8πG/c4)Tµv
I have several questions. what is the µv? when we use it today do we use the cosmological constant even though the universe isn't static or does it mean something different than einstein orignally thought? what are we measuring when we use this if theyre all constants?
 
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  • #2
I don't know the alt code either, but here's a copy-paster: Λ (from Wikipedia :))

The mu and nu are tensor indices, indicating that G, g and T are two-tensors. If you don't know what they are you should first of all learn about them, because they are very important constituents of the language in which GR is formulated (I recommend Carroll's book), but for now you can consider G, g and T as 4 x 4 matrices and mu, nu as simply indices, for example G00 is the top left component, etc.

The cosmological constant was written off a long time ago, but recently interest in it has arisen again. It can quite nicely explain some of the "odd" observed properties, such as the acceleration of the expansion rate of the universe and the fact that there seems to be more energy content than we'd expect. This might get you started, more advanced questions I will leave to the cosmologists out here :)
 
  • #3


The µv in this equation represents the indices of the metric tensor, which is a mathematical tool used to describe the curvature of spacetime. In simpler terms, it represents the four-dimensional coordinates of a point in spacetime.

In modern usage, the cosmological constant (Λ) is often included in the Einstein field equation to account for the observed expansion of the universe. This was not originally included in Einstein's theory, as he believed the universe to be static. However, it is now understood that the cosmological constant represents the energy density of empty space and can contribute to the overall curvature of spacetime.

When using this equation, we are essentially measuring the curvature of spacetime and how it is affected by the distribution of matter and energy (represented by Tµv). This allows us to understand how gravity works on a large scale and make predictions about the behavior of the universe. While the constants in the equation remain the same, the values of Tµv can vary depending on the specific situation being studied.
 

1. What is the Einstein field equation?

The Einstein field equation is a set of ten equations in Albert Einstein's theory of general relativity that describe the relationship between the curvature of space-time and the distribution of matter and energy.

2. How do the Einstein field equations relate to gravity?

The Einstein field equations are used to describe how the presence of mass and energy creates the curvature of space-time, which in turn determines the gravitational force between objects.

3. Can the Einstein field equations be applied to all types of matter and energy?

Yes, the Einstein field equations can be applied to any type of matter and energy, including both normal matter and exotic forms such as dark matter and dark energy.

4. Can the Einstein field equations be solved exactly?

No, the complete set of equations is highly complex and difficult to solve exactly. However, simplified versions of the equations can be used to make predictions that have been confirmed by various experiments and observations.

5. How have the Einstein field equations revolutionized our understanding of the universe?

The Einstein field equations have revolutionized our understanding of the universe by providing a more accurate and comprehensive theory of gravity. They have also helped to explain various phenomena, such as the bending of light by massive objects and the expansion of the universe. Furthermore, they have paved the way for advancements in fields such as cosmology and astrophysics.

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