2. Show that the Einstein equation \begin{equation} R_{\mu \nu} - \frac{1}{2} g_{\mu \nu} R + \Lambda g_{\mu \nu} = \frac{8 \pi G}{c^4} T_{\mu \nu} \quad (39) \end{equation} can be written in this alternative form: \begin{equation} R_{\mu \nu} = \frac{8 \pi G}{c^4} \left( T_{\mu \nu} - \frac{1}{2} T g_{\mu \nu} \right) + \Lambda g_{\mu \nu} \quad (40) \end{equation}
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Now, let's expand the Einstein tensor Gμν using its definition: Gμν = Rμν - 1/2 gμν R where Rμν is the Ricci tensor and R is the scalar curvature. Substituting this expression for Gμν back into the Einstein equation, we get: Rμν - 1/2 gμν R = 8πG Tμν Now, Show more…
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