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On the geodesic hypothesis in general relativity

In this paper, we give a rigorous derivation of Einstein's geodesic hypothesis in general relativity. We use scaling stable solitons for nonlinear wave equations to approximate the test particle. Given a vacuum spacetime $([0, T]\times\mathbb{R}^3, h)$, we consider the scalar field coupled Einstein equations. For all sufficiently small $ε$ and $δ\leq ε^q$, $q>1$, where $δ$, $ε$ are the amplitude and size of the particle, we show the existence of solution $([0, T]\times\mathbb{R}^3, g, ϕ^ε)$ to the coupled Einstein equations with the property that the energy of the particle $ϕ^ε$ is concentrated along a timelike geodesic. Moreover, the gravitational field produced by $ϕ^ε$ is negligibly small in $C^1$, that is, the spacetime metric $g$ is $C^1$ close to $h$. These results generalize those obtained by D. Stuart.