Contraction of the Riemann Tensor with the Weak Field Metric

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SUMMARY

The discussion focuses on the contraction of the Riemann tensor using a weak field metric defined by the equation ds²=-(1+2φ)dt²+(1-2φ)(dx²+dy²+dz²), where φ represents the gravitational potential. Participants derive the Christoffel symbols and subsequently compute various components of the Riemann tensor. A discrepancy arises when attempting to contract the Riemann tensor to find the Ricci tensor, specifically in the expression for R₀₀, which leads to confusion regarding the equivalence of φ^{,i}_{,i} and ∇²φ. The resolution confirms that these expressions are indeed equivalent, clarifying the misunderstanding.

PREREQUISITES
  • Understanding of weak gravitational fields and metrics
  • Familiarity with Christoffel symbols and their derivation
  • Knowledge of Riemann and Ricci tensors in general relativity
  • Proficiency in partial differentiation and the Laplacian operator
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  • Study the derivation of the Riemann tensor in general relativity
  • Learn about the properties and applications of the Ricci tensor
  • Explore the implications of weak field approximations in gravitational physics
  • Investigate the relationship between partial derivatives and the Laplacian operator in multiple dimensions
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Physicists, mathematicians, and students specializing in general relativity, particularly those interested in gravitational field theory and tensor calculus.

JMedley
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I have started with the space-time metric in a weak gravitational field (with the assumption of low velocity):
ds^2=-(1+2\phi)dt^2+(1-2\phi)(dx^2+dy^2+dz^2)
Where \phi<<1 is the gravitational potential. Using the standard form for the Christoffel symbols have found:
\Gamma^0_{00}=\phi_{,0}, \Gamma^0_{0i}=\Gamma^0_{i0}=\phi_{,i}, \Gamma^0_{ij}=\delta_{ij}\phi_{,0}
\Gamma^i_{00}=\phi^{,i}, \Gamma^i_{0j}=\Gamma^i_{j0}=-\delta^i_j\phi_{,0}, \Gamma^i_{jk}=\delta_{jk}\phi^{,i}-\delta^i_j\phi_{,k}-\delta^i_k\phi_{,j}
Then combining derivatives of these to first order (ignoring products of Christoffel symbols) using:
R^\alpha_{\beta\mu\nu}=\Gamma^\alpha_{\beta\nu,\mu} - \Gamma^\alpha_{\beta\mu,\nu}
to get:
R^0_{i0j}=\delta_{ij}\phi_{00}-\phi_{ij}, R^i_{0j0}=\phi^{,i}_{,j}+\delta^i_j\phi_{,00}
R^i_{0jk}=-\delta^i_k\phi_{,0j}+\delta^i_j\phi_{0k}, R^i_{kj0}=\delta^i_j\phi_{0k} - \delta_{jk}\phi^{,i}_{,0}
R^i_{kjl}=-\delta^i_l\phi_{,jk}+\delta_{kl}\phi^{,i}_{,j}+ {\delta^i_j}\phi_{,kl}-\delta_{jk}\phi^{,i}_{,l}
(Where greek indices run from 0 to 3 and latin indices run from 1 to 3, and commas denote coordinate partial differentiation). And here is where I run into problems.. When I try to use R_{\alpha\beta}=R^\sigma_{\alpha\sigma\beta} to contract these down to find the Ricci tensor. For example I get:
R_{00}=R^\sigma_{0\sigma 0}=\phi^{,i}_{,i}+\phi_{,00}
Which doesn't agree with the text I'm using which gives R_{00}=\nabla^2\phi +3\phi_{,00}
Can anybody spot where I'm going wrong? Many Thanks for any help.
Jack M
 
Last edited:
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Ri0j0,ijijϕ,00

When you contract this, don't forget that δii = 3.
 
Ok so that takes care of the factor 3, then how does \phi^{,i}_{,i} correspond to \nabla^2\phi? Cheers for the help
 
Last edited:
Because they are the same. I would assume that $\phi$ is a scalar (from what you showed) - then partial derivative is the same as the full derivative. And what you just wrote are exactly the same - just different way of expressing it. Hope it helps
 
JMedley said:
Ok so that takes care of the factor 3, then how does \phi^{,i}_{,i} correspond to \nabla^2\phi? Cheers for the help

You have \partial ^{i}\partial _{i}\phi = \delta ^{ij}\partial _{j}\partial _{i}\phi and this, in background flat 3 - space with a Cartesian chart is \delta ^{xx}\partial ^{2}_{x}\phi + \delta ^{yy}\partial ^{2}_{y}\phi + \delta ^{zz}\partial^{2} _{z}\phi = \partial ^{2}_{x}\phi + \partial ^{2}_{y}\phi + \partial^{2} _{z}\phi = \triangledown ^{2}\phi
 

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