For the given metric, the non-zero Christoffel symbols are
$$\frac{t_{\text{proper}}}{t_{\text{coordinate}}} = \sqrt{1 - \frac{2GM}{r}}$$ moore general relativity workbook solutions
where $L$ is the conserved angular momentum. For the given metric, the non-zero Christoffel symbols
Derive the geodesic equation for this metric. For the given metric