I Parallel transport general relativity

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Parallel transport of a tensor quantity in general relativity involves moving the tensor along a curve while maintaining its direction relative to the curve. In flat space, parallel transport is straightforward as the local reference frames at different points coincide. However, in curved spacetime, the final tensor coordinates after a closed path can differ from the initial ones due to the curvature, which affects the local reference frames. The choice of the curve does not dictate the local reference frames at each point but determines how the tensor is transported along the curve. Ultimately, the process illustrates that parallel transport is path-dependent in curved spaces, leading to different outcomes even when starting and ending at the same point.
  • #61
Jufa said:
If we state ##e_\theta=(1, 0) ## and ##e_\phi =(0, 1) ##

If ##e_\phi## is supposed to be a unit vector in the ##\phi## direction, then it is not ##(0, 1)##, it is ##(0, 1 / \sin \theta)##.
 
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  • #62
PeterDonis said:
If ##e_\phi## is supposed to be a unit vector in the ##\phi## direction, then it is not ##(0, 1)##, it is ##(0, 1 / \sin \theta)##.
I don't think it is a needed that the vectors are unitary. Indeed the only effect of choosing a non Unit vector in the basis is a change in the metric.
 
  • #63
Jufa said:
Actually we have ##e_\theta=(1, 0) ## and ##e_\phi =(0, 1) ## and the problem you point out is solved but the inconsestency remains.

You might be confusing yourself by switching equations too many times. Here's how I would work this problem using Equation 4.17 in the reference you gave earlier.

Equation 4.17 reads

$$
\frac{d A^\mu}{d \lambda} + \Gamma^\mu{}_{\nu \alpha} A^\alpha \frac{d x^\nu}{d \lambda} = 0
$$

Here the vector ##A^\mu## is ##e_\phi = (0, 1 / \sin \theta)##. Since our curve is the equator, we have ##\theta = \theta_0 = \pi / 2## all along the curve, and therefore ##d A^\mu / d \lambda = 0##. So we expect to find ##\Gamma^\mu{}_{\nu \alpha} A^\alpha \frac{d x^\nu}{d \lambda} = 0## for all possible index combinations.

Since ##A^1 = 0## (we have ##1## as the ##\theta## component index and ##2## as the ##\phi## component index), only ##\alpha = 2## needs to be considered. So the only connection coefficients that need to be considered are ##\Gamma^1{}_{22} = - \sin \theta \cos \theta## and ##\Gamma^2{}_{12} = \cot \theta##. Both of these vanish for ##\theta = \theta_0 = \pi / 2##. So Equation 4.17 is indeed satisfied for transporting ##e_\phi## along the equator.

Note that for other values of ##\theta## besides ##\pi / 2##, Equation 4.17 will not be satisfied for transporting ##e_\phi## along a curve of constant ##\theta##. That is because such curves are not geodesics for ##\theta \neq \pi / 2##.
 
  • #64
Jufa said:
As Romsofia suggested I tried to picture a simple example to see what's going on and I encounter something that I don't understand. Put this example: The surface of a sphere considereing the basis vectors as ## \vec{e_\theta} = \big(cos(\theta)cos(\phi), cos(\theta)sin(\phi), -sin(\theta)\big)## and ## \vec{e_\phi} = \big(-sin(\theta)sin(\phi), sin(\theta)cos(\phi), cos(\theta)\big)##.
The metric of this space is defined such that ##g_{11} = 1## and ##g_{22}=sin^2(\theta)## being zero the rest of the metric components and with the association ##\theta \rightarrow 1## and ##\phi\rightarrow 2##.

Let as now parallel transport the vector ##\vec{e_\phi}## from one point in the equator to another point on the equator, following the geodesic ##x^1=\theta_0## and ##x^2= \phi ##, being ##\theta_0## constant. The parallel transported vector, which we call ##\vec{v}##, must fulfill at every point the following:

$$\Big(\nabla_j \vec{v}\Big)^k \frac{dx^j}{d\phi} = 0 $$

We know that the solution is ##\vec{v} = \vec{e_\phi}## but if we insert this solution we get the following:

$$\Big(\nabla_j \vec{e_\phi}\Big)^k \frac{dx^j}{d\phi} = \Gamma^k_{j2} \frac{dx^j}{d\phi}= \Gamma^k_{22} $$

Where we have used that ##\frac{dx^j}{d\phi}=\delta^{j}_2##.
If we take k=1 we get:

$$\Big(\nabla_j \vec{v}\Big)^1 \frac{dx^j}{d\phi} = \Gamma^1_{22} = -\frac{1}{tg(\theta_0)}$$
which in general is different from zero.

Where am I wrong?
Oh. So Peter I think the result here is correct. I just needed to remember that ##\theta_0 =\pi/2##. Many thanks!
 

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