In D'Inverno's "Introducing Einstein's Relativity", an affine geodesic is defined as a privileged curve along which the tangent vector is propagated parallel to itself. Choosing an affine parameter, the affine geodesic equation reduces to
$$\frac{d^2x^a}{ds^2}+\Gamma^a_{bc}\frac{dx^b}{ds}\frac{dx^c}{ds}=0\tag{1}$$
Later, a metric is introduced, and a timelike metric geodesic is defined as a privileged curve that makes the interval $$s=\int_{P_1}^{P_2}\sqrt{g_{ab}\frac{dx^a}{du}\frac{dx^b}{du}}du\tag{2}$$ stationary under small variations. From Euler-Lagrange equations, and choosing a parameter $u$ which is linearly related to the interval $s$, the equation for a metric geodesic becomes
$$\frac{d^2x^a}{ds^2}+\frac 12 g^{ad}\left(\partial_cg_{bd}+\partial_bg_{cd}-\partial_dg_{bc}\right)\frac{dx^b}{ds}\frac{dx^c}{ds}=0.\tag{3}$$
Then, it states that once we have a manifold endowed with both an affine connection $\Gamma^a_{bc}$ and a metric, there are two classes of geodesics: affine ones and metric ones, which are different in general. However, if we take the metric connection
$$\Gamma^a_{bc}\equiv\frac 12 g^{ad}\left(\partial_cg_{bd}+\partial_bg_{cd}-\partial_dg_{bc}\right),\tag{4}$$
they will coincide. This definition leads to the identity $$\nabla_a g_{bc}=0\tag{5}$$ and, as $(4)$ is symmetric, the torsion is $0$.
Conversely, having a symmetric connection and requiring $(5)$ leads to the metric connection $(4)$.
My questions are:
- Why are we asking that both classes of geodesics coincide? What does it mean? Is there any physical motivation or is it general in differential geometry?
- Is it more natural to require this coincidence or that $\nabla_a g_{bc}=0$ and null torsion?
- In my lessons I was told that non-zero torsion has to be taken into account in quantum gravity theories . Without the goal of fully understanding why this is so, as it is still far from my knowledge, does it mean that metric geodesics and affine geodesics don't coincide in these theories?