Undergrad Reconciling 2 expressions for Riemann curvature tensor

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SUMMARY

This discussion focuses on reconciling two expressions for the Riemann curvature tensor as presented in Carroll's General Relativity notes. The coordinate-free definition (eq. 3.71) is given by $$R(X,Y)Z=\nabla_X\nabla_YZ-\nabla_Y\nabla_XZ-\nabla_{[X,Y]}Z$$ while the index-based expression (eq. 3.66) is $$R^{\rho}_{\ \ \sigma\mu\nu}V^{\sigma}=[\nabla_{\mu},\nabla_{\nu}]V^{\rho}+T_{\mu\nu}^{\ \ \ \ \lambda}\nabla_{\lambda}V^{\rho}$$. The participants emphasize the importance of understanding the non-commutativity of vector fields and the implications of torsion in the context of these equations. They also highlight the necessity of using appropriate vectors that do not commute for accurate comparisons.

PREREQUISITES
  • Understanding of Riemann curvature tensor and its definitions
  • Familiarity with covariant derivatives and the notation used in differential geometry
  • Knowledge of torsion tensors and their implications in General Relativity
  • Ability to manipulate and interpret tensor equations in both coordinate-free and index-based forms
NEXT STEPS
  • Study the properties of the Riemann curvature tensor in detail, focusing on its coordinate-free definition
  • Learn about the implications of torsion in non-standard connections in General Relativity
  • Explore the differences between covariant derivatives and their applications in tensor calculus
  • Review the treatment of curvature in "Gravitation" by Misner, Thorne, and Wheeler for a comprehensive understanding
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Students and researchers in theoretical physics, particularly those studying General Relativity, differential geometry, or tensor calculus, will benefit from this discussion.

  • #31
PeterDonis said:
The whole calculation is wrong because it's based on a wrong assumption: that you can obtain Carroll's equation 3.66 by applying the Riemann curvature tensor to general (non-commuting) vector fields. You can't. You obtain Carroll's Equation 3.66 by applying the Riemann curvature tensor to coordinate basis vector fields only.
(Hope I don't sound argumentative, it's just that I always try to get full clarity) So a couple of points:
  1. I was asking about calculation on a standalone basis (the calculation itself doesn't refer to Carroll's equation) - look at it as a generic differential geometry calculation. I'm not sure if (and where) I've gone wrong in that
  2. The identity is a result on second order covariant derivatives and the definition is that of a total covariant derivative. Both can be found in Lee's Introduction to Riemannian Manifolds (resp. Proposition 4.21 and Proposition 4.17)
 
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  • #32
Shirish said:
I was asking about calculation on a standalone basis
Then I don't understand what you are trying to show with the calculation. I also don't understand what in Carroll you are trying to compare it to, if it isn't Equation 3.66.

(I note, btw, that while you use general vectors ##X##, ##Y##, and ##Z##, you use the coordinate basis vector ##\partial_\rho## instead of a general covector. You should use a general covector.)
 
  • #33
PeterDonis said:
Then I don't understand what you are trying to show with the calculation.
So the calculation shows that $$X^{\mu}Y^{\nu}Z^{\sigma}R^{\rho}_{\ \ \sigma\mu\nu}\partial_{\rho}=X^{\mu}Y^{\nu}\big(T_{\mu\nu}^{\ \ \ \ \lambda}(\nabla_{\partial_{\lambda}}Z)^{\rho}+\nabla^2Z(\text{d}x^{\rho},\partial_{\nu},\partial_{\mu})-\nabla^2Z(\text{d}x^{\rho},\partial_{\mu},\partial_{\nu})\big)\partial_{\rho}$$
$$\implies X^{\mu}Y^{\nu}\big(Z^{\sigma}R^{\rho}_{\ \ \sigma\mu\nu}\big)\partial_{\rho}=X^{\mu}Y^{\nu}\big(T_{\mu\nu}^{\ \ \ \ \lambda}(\nabla_{\partial_{\lambda}}Z)^{\rho}+\nabla^2Z(\text{d}x^{\rho},\partial_{\nu},\partial_{\mu})-\nabla^2Z(\text{d}x^{\rho},\partial_{\mu},\partial_{\nu})\big)\partial_{\rho}$$
$$\implies Z^{\sigma}R^{\rho}_{\ \ \sigma\mu\nu}=T_{\mu\nu}^{\ \ \ \ \lambda}(\nabla_{\partial_{\lambda}}Z)^{\rho}+\nabla^2Z(\text{d}x^{\rho},\partial_{\nu},\partial_{\mu})-\nabla^2Z(\text{d}x^{\rho},\partial_{\mu},\partial_{\nu})$$ and this is what I was trying to compare to Carroll's eq. 3.66
 
  • #34
Shirish said:
So the calculation shows that $$X^{\mu}Y^{\nu}Z^{\sigma}R^{\rho}_{\ \ \sigma\mu\nu}\partial_{\rho}=X^{\mu}Y^{\nu}\big(T_{\mu\nu}^{\ \ \ \ \lambda}(\nabla_{\partial_{\lambda}}Z)^{\rho}+\nabla^2Z(\text{d}x^{\rho},\partial_{\nu},\partial_{\mu})-\nabla^2Z(\text{d}x^{\rho},\partial_{\mu},\partial_{\nu})\big)\partial_{\rho}$$
$$\implies X^{\mu}Y^{\nu}Z^{\sigma}\big(R^{\rho}_{\ \ \sigma\mu\nu}\big)\partial_{\rho}=X^{\mu}Y^{\nu}\big(T_{\mu\nu}^{\ \ \ \ \lambda}(\nabla_{\partial_{\lambda}}Z)^{\rho}+\nabla^2Z(\text{d}x^{\rho},\partial_{\nu},\partial_{\mu})-\nabla^2Z(\text{d}x^{\rho},\partial_{\mu},\partial_{\nu})\big)\partial_{\rho}$$
$$\implies R^{\rho}_{\ \ \sigma\mu\nu}=T_{\mu\nu}^{\ \ \ \ \lambda}(\nabla_{\partial_{\lambda}}Z)^{\rho}+\nabla^2Z(\text{d}x^{\rho},\partial_{\nu},\partial_{\mu})-\nabla^2Z(\text{d}x^{\rho},\partial_{\mu},\partial_{\nu})$$ and this is what I was trying to compare to Carroll's eq. 3.66
You still do not get it. It makes no sense to compare what you calculated with Carroll's Equation 3.66. I have already explained why several times. There is no point in explaining it again. You are evidently on a fool's errand and you are not listening when I try to explain that.
 
  • #35
The OP question is based on a misunderstanding, which has been repeatedly explained. Enough is enough. Thread closed.
 

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