Metric Tensor Components: Inverse & Derivatives

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SUMMARY

The discussion focuses on the metric tensor components in General Relativity (GR), specifically the weak field approximation where the metric tensor is expressed as g_{\mu \nu} = \eta_{\mu \nu} + h_{\mu \nu} with |h| << 1. The inverse metric tensor is approximated as g^{\mu \nu} = \eta^{\mu \nu} - h^{\mu \nu}, although this does not yield the identity g^{\mu \rho}g_{\rho \nu} = \delta^{\mu}_{\nu} due to the presence of the term -h^{\mu \rho}h_{\rho \nu}. Additionally, the derivatives of h are treated similarly to h itself, leading to terms like h ∂h and ∂h ∂h being of order \mathcal{O}(h^2).

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ChrisVer
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I have one question, which I don't know if I should post here again, but I found it in GR...
When you have a metric tensor with components:
g_{\mu \nu} = \eta _{\mu \nu} + h_{\mu \nu}, ~~ |h|&lt;&lt;1 (weak field approximation).

Then the inverse is:

g^{\mu \nu} = \eta^{\mu \nu} - h^{\mu \nu} right? However that doesn't give exactly that g^{\mu \rho}g_{\rho \nu} = \delta^{\mu}_{\nu} because of the existence of the - h^{\mu \rho}h_{\rho \nu} which is of course small but it's not zero... Can the inverse matrix be defined approximately?

Also I don't understand why should the derivatives of h behave as h itself? I mean they take the terms like h \partial h, ~~ \partial h \partial h to be of order \mathcal{O}(h^2)... why?
 
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They mean to write
g_{ \mu \nu } = \eta_{ \mu \nu } + \epsilon h_{ \mu \nu } , \ \ \ |\epsilon | \ll 1.
Then all the following holds
g \cdot g = \delta + \mathcal{O}( \epsilon^{2} ) , \ \ h \cdot h \sim h \partial h \sim \partial h \cdot \partial h \sim \mathcal{O} ( \epsilon^{ 2 } ) .
 
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