As is well known Newton's laws:
$$m\frac{\text{d}^2 x_i}{\text{d}t^2} = F_i$$
whose relativistic generalization is:
$$m \left(\frac{\text{d}^2 x^\mu}{\text{d}\tau^2} + \sum_{\sigma,\nu} \Gamma_{\sigma \nu}^{\mu} \frac{\text{d} x^\sigma}{\text{d}\tau}\frac{\text{d} x^\nu}{\text{d}\tau}\right) = F^\mu$$
only work in an inertial reference system, in a non-inertial system additional fictitious forces appear, which in the relativistic case translate into the Christoffel symbols are not to be identically null $\Gamma_{\sigma \nu}^{\mu} \neq 0$.
In principle, Larmor's formula for the radiated energy:
$$ \frac{\text{d}E}{\text{d}t} = \frac{q^2 a^2}{6 \pi \varepsilon_0 c^3} $$
provides a method for an inertial observer to detect relative accelerations: an observer could notice that his system is not inertial if by placing a sufficiently large charge he is able to detect the electromagnetic radiation emitted by it (in the quantum context this leads to the Unruh effect).
My doubt is the following, in relativity theory it is said that an observer is inertial if its Christoffel symbols cancel out, but on the other hand an electric charge falling in a gravitational field describes a coordinate system with null Christoffel symbols, but still that charge emits radiation because the curvature of spacetime deforms its electric field and as a consequence that charge emits radiation, even being in an "inertial system". Therefore, we have two non-equivalent definitions of inertial system in relativity:
- An observer in whose coordinate system the Christoffel symbols cancel out.
- An observer who sees an electric charge at rest with respect to him does not emit radiation.
Which of these two definitions seems more appropriate to identify a non-inertial system?