Riemann tensor and derivatives of ##g_{\mu\nu}##

In summary, the Riemann tensor cannot depend on ##g_{\mu\nu}## and its first derivatives alone because in a curved spacetime, there is always a coordinate system in which the first derivatives of the metric tensor vanish, but the second derivatives do not. This means that the desired tensor must be equal to one constructed solely from the metric tensor, but this only holds at a single point in a locally inertial frame. In other points and frames, the tensor will be different.
  • #1
Einj
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Hello everyone,
I'm studying Weinberg's 'Gravitation and Cosmology'. In particular, in the 'Curvature' chapter it says that the Riemann tensor cannot depend on ##g_{\mu\nu}## and its first derivatives only since:

... at any point we can find a coordinate system in which the first derivatives of the metric tensor vanish, so in this coordinate system the desired tensor must be equal to one of those that can be constructed out of the metric tensor alone, ..., and since this is an equality between tensors it must be true in all coordinate systems.

What I don't understand is how introducing the second derivatives should change this situation. The point is that (and I'm not sure about that...) we can always find a locally inertial frame. In this frame ##g_{\mu\nu}=\eta_{\mu\nu}##, which is constant, and hence all its derivatives should vanish.
What am I doing wrong?

Thanks a lot
 
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  • #2
The wrong part of your reasoning is that only if spacetime is flat, you can find a coordinate system in which [itex] g_{\mu\nu}=\eta_{\mu\nu} [/itex] globally. In a curved spacetime, its only that there is always a coordinate system that at a given point P, [itex] g_{\mu \nu}(x_p)=\eta_{\mu \nu} [/itex]. The first derivatives at P can be made to vanish too but not the second derivatives.
 
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  • #3
Einj said:
In this frame ##g_{\mu\nu}=\eta_{\mu\nu}##, which is constant, and hence all its derivatives should vanish.

You left out a key qualifier: in the local inertial frame, ##g_{\mu \nu} = \eta_{\mu \nu}## at a single point (the origin of the frame). At other points, ##g_{\mu \nu} \neq \eta_{\mu \nu}##.
 
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  • #4
It makes perfect sense! Thanks a lot!
 
  • #5
If you ever get confused on this again, just think about the function ##f(x)=x^2##. The first derivative of this function ##f'(x)=2x## vanishes at ##x=0## but the second derivative ##f''(x)=2## does not. The first derivative measures a slope, while the second derivative measures concavity - which is roughly analogous to curvature.
 

Related to Riemann tensor and derivatives of ##g_{\mu\nu}##

1. What is the Riemann tensor?

The Riemann tensor is a mathematical object that describes the curvature of a Riemannian manifold. It is defined as a set of numbers that represent the change in direction of a vector as it is parallel transported around a closed loop on the manifold.

2. What are the derivatives of ##g_{\mu\nu}##?

The derivatives of ##g_{\mu\nu}## refer to the partial derivatives of the metric tensor with respect to its indices. These derivatives are used to calculate the components of the Riemann tensor and other curvature tensors.

3. How are the Riemann tensor and metric tensor related?

The Riemann tensor is constructed from the derivatives of the metric tensor. It is a combination of the second derivatives of the metric tensor that represents the intrinsic curvature of the manifold.

4. What is the significance of the Riemann tensor in general relativity?

The Riemann tensor is a key component in the mathematical formulation of general relativity. It describes the curvature of spacetime, which is directly related to the distribution of matter and energy. In general relativity, this curvature is what determines the motion of massive objects and the behavior of light.

5. Are there any alternative formulations of the Riemann tensor?

Yes, there are alternative formulations of the Riemann tensor, such as the Weyl tensor and the Ricci tensor. These tensors have different properties and can be used to describe different aspects of curvature on a manifold. However, the Riemann tensor is the most commonly used and fundamental tensor in general relativity.

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