Riemann curvature tensor derivation

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Discussion Overview

The discussion centers around the derivation of the Riemann curvature tensor, exploring the mathematical formulation and conceptual understanding of curvature in the context of geodesics and covariant derivatives. Participants examine the relationship between the commutator of covariant derivatives and the Riemann tensor, as well as the implications of curvature on the behavior of geodesics.

Discussion Character

  • Technical explanation
  • Conceptual clarification
  • Mathematical reasoning

Main Points Raised

  • Some participants describe the calculation of the Riemann curvature tensor as involving the commutator of covariant derivatives, questioning why this antisymmetry leads to the Riemann tensor.
  • Others elaborate on the role of basis vectors and the geometric interpretation of curvature, suggesting that the change in a vector carried around a small quadrilateral reflects the curvature of the space.
  • A participant explains that the Riemann tensor quantifies the acceleration between two parallel geodesics, detailing how to compute the difference in their accelerations using the affine parameter.
  • Another participant reiterates the connection between the Riemann tensor and the change in separation of geodesics in curved space, emphasizing the tensor's emergence from differences in acceleration.
  • One participant shares a link to a resource they found helpful for understanding the derivation, indicating that they have found clarity in the topic.

Areas of Agreement / Disagreement

Participants express varying levels of understanding and interpretation regarding the derivation of the Riemann curvature tensor. There is no consensus on a single explanation, as multiple perspectives and methods of reasoning are presented.

Contextual Notes

Some participants acknowledge uncertainty in their understanding and express the possibility of being incorrect in their interpretations. The discussion includes complex mathematical expressions and assumptions that may not be fully resolved.

weio
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Hey,

when calculating the Riemann curvature tensor, you need to calculate the commutator of some vector field [tex]V[/tex], ie like this :-

[tex][\bigtriangledown_a, \bigtriangledown_b][/tex] = [tex]\bigtriangledown_a\bigtriangledown_b - \bigtriangledown_b\bigtriangledown_a[/tex] = [tex]V;_a_b - V;_b_a[/tex]

But why does this difference of antisymmtery give us the Riemman tensor?

thanks
 
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weio said:
Hey,

when calculating the Riemann curvature tensor, you need to calculate the commutator of some vector field [tex]V[/tex], ie like this :-

[tex][\bigtriangledown_a, \bigtriangledown_b][/tex] = [tex]\bigtriangledown_a\bigtriangledown_b - \bigtriangledown_b\bigtriangledown_a[/tex] = [tex]V;_a_b - V;_b_a[/tex]

But why does this difference of antisymmtery give us the Riemman tensor?

thanks

In addition to the commutator of the covariant derivatives, you need the commutator of the basis vectors too. Ignore torsion.

Think of your covariant derivative as a change along your basis. In a coordinate basis (defined by vanishing basis commutators) two different basis vectors span a plane. Think of a small quadrilateral spanned by the two basis vectors. When the vector V is carried around this quadrilateral your commutator of covariant derivatives gives the change in V. It's length can't change, but its direction does. So with R the full Riemann curvature:
[grada , gradb] V = R(.,V,a,b) . Riemann set up his geometry so it would look flat in the small. However, he was amazed that this difference resulting from taking a vector to nearby points could be described by an object (the full curvature tensor) that lived solely at the base point. This made him realize the importance of the curvature tensor and gave substance to his geometry.
 
Hey

So far this is how I understand it, though I know I could be very wrong. If you have two geodesics parallel to each other, with tangents [tex]V[/tex] and [tex]V'[/tex] , in which the coordinate [tex]x^\alpha[/tex] point along both geodesics. There is some connecting vector [tex]w^\alpha[/tex] between them. Let the affine parameter on the geodesics be [tex]\lambda[/tex]

Riemman tensor calculates the acceleration between these two geodesics. so you calculate the acceleration at some point A, A' on each geodesic , and subtract them. this gives you an expression telling how the components of [tex]w^\alpha[/tex] change.

[tex]\frac{d^2w^\alpha} {d\lambda^2} = \frac{d^2x^\alpha} {d\lambda^2} | A' - \frac {d^2x^\alpha} {d\lambda^2} | A = - \Gamma^\alpha_0_0_\beta w^\beta[/tex]

After that you calculate the full 2nd covariant derivative along V, ie , you get something like
[tex]\bigtriangledown v \bigtriangledown v w^\alpha = (\Gamma^\alpha_\beta_0_0 - \Gamma^\alpha_0_0,\beta) w^\beta[/tex]
[tex]= R^a_0_0\beta w^\beta[/tex]
[tex]= R^a_u_v_\beta V^u V^v w^\beta[/tex]

That's where the tensor arises. so basically it's a difference in acceleration as geodesics don't maintain their separation in curved space.
 
weio said:
Hey

So far this is how I understand it, though I know I could be very wrong. If you have two geodesics parallel to each other, with tangents [tex]V[/tex] and [tex]V'[/tex] , in which the coordinate [tex]x^\alpha[/tex] point along both geodesics. There is some connecting vector [tex]w^\alpha[/tex] between them. Let the affine parameter on the geodesics be [tex]\lambda[/tex]

Riemman tensor calculates the acceleration between these two geodesics. so you calculate the acceleration at some point A, A' on each geodesic , and subtract them. this gives you an expression telling how the components of [tex]w^\alpha[/tex] change.

[tex]\frac{d^2w^\alpha} {d\lambda^2} = \frac{d^2x^\alpha} {d\lambda^2} | A' - \frac {d^2x^\alpha} {d\lambda^2} | A = - \Gamma^\alpha_0_0_\beta w^\beta[/tex]

After that you calculate the full 2nd covariant derivative along V, ie , you get something like
[tex]\bigtriangledown v \bigtriangledown v w^\alpha = (\Gamma^\alpha_\beta_0_0 - \Gamma^\alpha_0_0,\beta) w^\beta[/tex]
[tex]= R^a_0_0\beta w^\beta[/tex]
[tex]= R^a_u_v_\beta V^u V^v w^\beta[/tex]

That's where the tensor arises. so basically it's a difference in acceleration as geodesics don't maintain their separation in curved space.

Yes it arises there and in many other places, including the one you asked about and that I told you about.
 
Thanks!

I understand the derivation now. I found a simple one which fully explains it. for the curious, here is the link :- http://www.anasoft.co.uk/physics/gr/reimann/reimann.html

weio
 
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