Contravariant metric components

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SUMMARY

The discussion focuses on expanding the contravariant metric tensor components g^{\mu\nu} in terms of the covariant metric tensor g_{\mu\nu}, particularly up to second order. The user employs the equations g^{\lambda\mu}g_{\mu\sigma} = \delta^\lambda_\sigma and g^{\mu\nu} \equiv \eta^{\mu\nu} + \sqrt{G}*h^{\mu\nu} to derive the expansion. The challenge lies in the increasing complexity and number of terms in the expansion as the order increases, making the second order calculation tedious. The user seeks either a direct solution or a reference to existing resources on this topic.

PREREQUISITES
  • Understanding of tensor calculus, specifically contravariant and covariant tensors.
  • Familiarity with the metric tensor and its properties in general relativity.
  • Knowledge of perturbation methods in quantum gravity.
  • Proficiency in mathematical manipulation of series expansions and matrix forms.
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  • Research the derivation of the contravariant metric tensor from the covariant metric tensor in general relativity.
  • Study perturbative approaches in quantum gravity, focusing on metric perturbations.
  • Explore existing literature on tensor expansions and their applications in theoretical physics.
  • Investigate computational tools or algorithms for simplifying tensor calculations in higher orders.
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The discussion is beneficial for theoretical physicists, mathematicians, and researchers working in the fields of general relativity and quantum gravity, particularly those dealing with tensor analysis and metric expansions.

michael879
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I realize this is a "simple" mathematical exercise, in theory, but I'm having a lot of trouble finding some algorithmic way to do it. The problem is this: I want to expand the contravariant metric tensor components g^{\mu\nu} in terms of the covariant metric tensor g_{\mu\nu}. The first order calculation is very simple, but the second order one seems incredibly tedious and error prone. Could someone either show me this expansion to at least 2nd order or direct me to a source that does? I'm trying to do some stuff with quantum gravity and I don't want to spend all this time on such a trivial problem if the answer is already out there (I have looked).

Also, here is the method I have been using:
g^{\lambda\mu}g_{\mu\sigma} = \delta^\lambda_\sigma
g^{\mu\nu} \equiv \eta^{\mu\nu} + sqrt(G)*h^{\mu\nu}
g_{\mu\nu} \equiv \eta_{\mu\nu} + sqrt(G)*h_{\mu\nu}

and then just use the resulting formula to calculate the contravariant h in terms of the covariant h order by order (use all possible combinations of h, \eta, and \partial for each order of h and assign some constant that will be solved for). The problem is that the number of terms at each order grows very fast.
 
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Let's do it in matrix form first and then put the indices in. Let N = ημν, H = hμν, and G = gμν.

G = (N + H)-1 = ((I + HN-1)N)-1 = N-1(I + HN-1)-1 = N-1 - N-1HN-1 + N-1HN-1HN-1 + ...

Therefore

gμν = ημν - ημαhαβηβν + ημαhαβηβγhγεηεν + ...
 
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In an inertial frame of reference (IFR), there are two fixed points, A and B, which share an entangled state $$ \frac{1}{\sqrt{2}}(|0>_A|1>_B+|1>_A|0>_B) $$ At point A, a measurement is made. The state then collapses to $$ |a>_A|b>_B, \{a,b\}=\{0,1\} $$ We assume that A has the state ##|a>_A## and B has ##|b>_B## simultaneously, i.e., when their synchronized clocks both read time T However, in other inertial frames, due to the relativity of simultaneity, the moment when B has ##|b>_B##...

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