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Contraction of the Riemann Tensor with the Weak Field Metric

  1. Sep 19, 2011 #1
    I have started with the space-time metric in a weak gravitational field (with the assumption of low velocity):
    [tex] ds^2=-(1+2\phi)dt^2+(1-2\phi)(dx^2+dy^2+dz^2)[/tex]
    Where [tex]\phi<<1[/tex] is the gravitational potential. Using the standard form for the Christoffel symbols have found:
    [tex] \Gamma^0_{00}=\phi_{,0}, \Gamma^0_{0i}=\Gamma^0_{i0}=\phi_{,i}, \Gamma^0_{ij}=\delta_{ij}\phi_{,0}[/tex]
    [tex] \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} [/tex]
    Then combining derivatives of these to first order (ignoring products of Christoffel symbols) using:
    [tex] R^\alpha_{\beta\mu\nu}=\Gamma^\alpha_{\beta\nu,\mu} - \Gamma^\alpha_{\beta\mu,\nu} [/tex]
    to get:
    [tex] R^0_{i0j}=\delta_{ij}\phi_00-\phi_{ij}, R^i_{0j0}=\phi^{,i}_{,j}+\delta^i_j\phi_{,00} [/tex]
    [tex] 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} [/tex]
    [tex] R^i_{kjl}=-\delta^i_l\phi_{,jk}+\delta_{kl}\phi^{,i}_{,j}+ {\delta^i_j}\phi_{,kl}-\delta_{jk}\phi^{,i}_{,l} [/tex]
    (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 [tex] R_{\alpha\beta}=R^\sigma_{\alpha\sigma\beta} [/tex] to contract these down to find the Ricci tensor. For example I get:
    [tex] R_{00}=R^\sigma_{0\sigma 0}=\phi^{,i}_{,i}+\phi_{,00} [/tex]
    Which doesn't agree with the text I'm using which gives [tex] R_{00}=\nabla^2\phi +3\phi_{,00} [/tex]
    Can anybody spot where I'm going wrong? Many Thanks for any help.
    Jack M
     
  2. jcsd
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