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+2 votes

Let's use the Schwarzschild spacetime notebook as an example, using these lines:

{r,t,\phi,\theta}::Coordinate; 
{\mu,\nu,\rho,\sigma,\lambda,\kappa,\chi,\gamma}::Indices(values={t,r,\phi,\theta}, position=fixed);
\partial{#}::PartialDerivative; 
g_{\mu\nu}::Metric. 
g^{\mu\nu}::InverseMetric.
ss:= { g_{t t} = -(1-2 M/r), g_{r r} = 1/(1-2 M/r), g_{\theta\theta} = r**2, g_{\phi\phi}=r**2 sin(\theta)**2 }. 
complete(ss, $g^{\mu\nu}$);

So, we have gμν and gμν completely determined and we should be able to explicitly calculate its determinant and trace. How would one do it properly in Cadabra?

in General questions by (180 points)

1 Answer

+2 votes
 
Best answer

There's a Determinant property now which you can use together with complete to compute determinants, as in https://cadabra.science/manual/Determinant.html .

by (84.8k points)
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How to calculate trace?

In the same way, e.g. in the above example

T::Trace(g_{m n});
complete(rl, $T$);

Note that this traces over lower indices (a trace over mixed indices would produce the dimension '3').

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