Can geodesic deviation be zero while curvature tensor is not

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SUMMARY

Geodesic deviation describes the divergence or convergence of parallel geodesics on manifolds, serving as a specific application of the Riemann curvature tensor. While geodesic deviation provides insights into curvature, it is not equivalent to the full description offered by the Riemann curvature tensor, which encompasses broader cases. The geodesic deviation equation, represented as D²J/dt² = -R(J(t),c'(t))c'(t), relates to sectional curvature in Riemannian manifolds, indicating that geodesic deviations can reveal significant information about the curvature tensor. However, the situation is more complex in Lorentzian manifolds due to the presence of degenerate planes.

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  • Understanding of Riemann curvature tensor
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Elnur Hajiyev
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I understand(or assume understand) that geodesic deviation describes how much parallel geodesics diverge/converge on manifolds while moving along these geodesic. But is not it a definition for intrinsic curvature? If it is same as Riemann curvature tensor in terms of describing curvature, why there is two distinct notion to describe it?

Thanks.
 
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Elnur Hajiyev said:
I understand(or assume understand) that geodesic deviation describes how much parallel geodesics diverge/converge on manifolds while moving along these geodesic. But is not it a definition for intrinsic curvature? If it is same as Riemann curvature tensor in terms of describing curvature, why there is two distinct notion to describe it?

Thanks.

Geodesic deviation is a special case of applying the Riemann curvature tensor.

The informal meaning of the curvature tensor is this:

Make a "rectangle" with sides given by vectors U^\mu and V^\mu. Take a third vector W^\mu, and parallel-transport it around the rectangle to get back to the start. Then the change in W^\mu resulting from the parallel-transport is:

\delta W^\mu = R^\mu_{\nu \lambda \sigma} W^\nu U^\lambda V^\sigma

Geodesic deviation only gives you information about the special case in which W = V; the vector that you are parallel-transporting around the rectangle is the separation vector between the sides of the rectangle.
 
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I am not sure about Lorentzian manifolds but for Riemannian manifolds the entire Riemann curvature tensor is determined by the sectional curvatures of tangential 2 planes.

These are the normalized curvatures ,##<R(X,Y)Y,X>/<X,X><Y,Y> - <X,Y>^2##.

The geodesic deviation equation ##D^2J/dt^2 = - R(J(t),c'(t))c'(t)## almost gives you the sectional curvature of the 2 plane spanned by ##J(t)## and ##c'(t)##. One only needs to take the inner product with ##J## and normalize. So for a Riemannian manifold one ought to be able to determine the entire curvature tensor from geodesic deviations. ( Note that sectional curvature is not defined for a degenerate 2 plane on a Lorentzian manifold.)

The variation vector field of a variation through geodesics is always a Jacobi field. That is: it always satisfies the geodesic deviation equation. One can always find a variation through geodesics that has an arbitrary Jacobi field as its variation vector field. This means that one can always compute ##R(J(t),c'(t))c'(t)## at any point along the geodesic in terms of some variation through geodesics. So for a Riemannian manifold the answer to your question is yes.

For a Lorentzian manifold I am not sure since there are degenerate 2 planes. Also the proof that every Jacobi field is the variation vector field of a variation through geodesics depends on the existence of a neighborhood of each point where each point is connected by a unique minimal geodesic. I tried to find a reference on line but without luck. I am sure one of the Relativity experts here would know the answer. In any case, the geodesic deviations ought to tell you a lot about the curvature tensor if not the whole thing. I would be interested to know the answer.
 
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