Riemann tensor in normal coordinates (General Relativity)

In summary, the Riemann tensor can be simplified to just the derivatives of the connection terms in normal coordinates. This solution, although seemingly simple, is correct and demonstrates a good understanding of the topic. It also shows the use of normal coordinates to simplify the calculation of the Riemann tensor.
  • #1
alcoholicsephiroth
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Homework Statement



Find a simplified expression for the Riemann tensor in terms of the connection in normal coordinates.

Homework Equations



Riemann tensor = (derivative of connection term) - (derivative of connection term) - (connection term)(connection term) - (connection term)(connection term)

The Attempt at a Solution



My solution is

Riemann tensor = (derivative of connection term) - (derivative of connection term)

, where I have used the fact that the connections evaluated at point P are all 0, but their derivatives are not necessarily 0.

My problem is that 3 MARKS are allocated to this question (from a possible 60 marks in a 2 hour paper), and that this looks far too simple a solution for 3 marks.

What am I missing?

Trev
 
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  • #2
or, your solution is correct and it is not too simple for 3 marks. The Riemann tensor is a 4-dimensional object and its calculation involves a lot of terms and calculations. By simplifying it to just the derivatives of the connection terms, you have already done a significant amount of work and demonstrated a good understanding of the topic. Your solution is concise and shows that you know how to use normal coordinates to simplify the Riemann tensor. Keep up the good work!
 

Related to Riemann tensor in normal coordinates (General Relativity)

1. What is the Riemann tensor in normal coordinates?

The Riemann tensor in normal coordinates is a mathematical object used in the study of general relativity. It represents the curvature of spacetime at a given point and is defined by a set of 20 components that describe how the metric tensor changes as you move through space.

2. How is the Riemann tensor in normal coordinates related to general relativity?

The Riemann tensor in normal coordinates is a fundamental tool in the study of general relativity. It allows us to calculate the curvature of spacetime, which is a key concept in Einstein's theory of gravity. By understanding the Riemann tensor, we can better understand the effects of mass and energy on the fabric of spacetime.

3. What are the applications of the Riemann tensor in normal coordinates?

The Riemann tensor in normal coordinates has a wide range of applications in general relativity, including calculating the trajectories of particles in curved spacetime, predicting the behavior of light in the presence of massive objects, and determining the gravitational force between two bodies. It is also used in the study of black holes and cosmology.

4. How is the Riemann tensor in normal coordinates calculated?

The Riemann tensor in normal coordinates is calculated using the Christoffel symbols, which describe the connection between the metric tensor and the coordinates used to describe a curved space. These symbols are used to calculate the components of the Riemann tensor, which can then be used to analyze the curvature of spacetime at a given point.

5. What are the limitations of the Riemann tensor in normal coordinates?

While the Riemann tensor in normal coordinates is a powerful tool in the study of general relativity, it does have some limitations. It is only valid in the context of a smooth, continuous spacetime, and it cannot be used to describe the behavior of matter at a quantum level. Additionally, it assumes that the metric tensor is continuous and differentiable, which may not always be the case in extreme gravitational environments.

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