Is the Contravariant Derivative Defined by Contracting with the Metric?

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The discussion revolves around the definition and calculation of the contravariant derivative, specifically v^a;b, in the context of general relativity. It clarifies that v^{a;b} can be obtained by contracting the covariant derivative v^a _;b with the metric tensor, g^{bc}, to raise the indices. The term "covariant" refers to the transformation properties of tensor components under coordinate changes, emphasizing the need for a covariant derivative to ensure physical laws are tensorial. The conversation also touches on the importance of the connection in defining the covariant derivative and its relation to local symmetries in physics. Understanding these concepts is crucial for proper tensor manipulation in general relativity.
Pacopag
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Hi everyone;
I'm new to both PF and GR, so please bear with me if I'm not being very clear, or using standard syntax and such. Here is my question.

Given a vector v^a, the covariant derivative is defined as v^a _;b = v^a _,b + v^c GAMMA^a _bc.
(here I'm using ^ before upper indices and _ before lower indices).
The object I'm interested in now is v^a;b (where the whole thing a;b is upper). Is this called the contravariant derivative? Is there a similar definition in terms of the Christoffel symbol? or can we only obtain it from contracting v^a _;b with the metric? I can't seem to find the definition of this object in any books, and when I try to do my calculation via contraction with the metric, I'm getting the wrong answer.

Thanks.
 
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You might want to look at the Latex capabilities of PF. Quote this post for examples.

The short answer is that you should already know how to or be able to find out how to raise and lower indices with tensors. Then

v^{a;b} = g^{bc} v^a{}_{;c}
 
Ok. Thanks pervect.
 
The term "covariant" is used in the sense of how the components of a tensor transform. But covariance also means that the laws of physics can be written down tensorially, and so have a certain behaviour under coordinate transformations.

The covariant derivative is the demand that we use a derivative in our physical formulation that transforms tensorially. The partial derivative doesn't, so we need an extra term. This is the connection, but to specify it you have to demand certain properties on it. The same happens in the standard model: you impose a local symmetry, and demand that the derivative of your fields transforms exactly as the field itself under the symmetry transformation.
 
In an inertial frame of reference (IFR), there are two fixed points, A and B, which share an entangled state $$ \frac{1}{\sqrt{2}}(|0>_A|1>_B+|1>_A|0>_B) $$ At point A, a measurement is made. The state then collapses to $$ |a>_A|b>_B, \{a,b\}=\{0,1\} $$ We assume that A has the state ##|a>_A## and B has ##|b>_B## simultaneously, i.e., when their synchronized clocks both read time T However, in other inertial frames, due to the relativity of simultaneity, the moment when B has ##|b>_B##...

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