Critique of the use of geodesics in astrophysics and cosmology
Philip D. Mannheim

TL;DR
This paper critically examines the assumption that particles follow geodesics in astrophysics and cosmology, showing that wave-based propagation often deviates from geodesic paths, especially in curved spacetime, with implications for gravitational lensing and light behavior.
Contribution
The study demonstrates that wave equations do not generally lead to geodesic trajectories in curved spacetime, challenging the standard null geodesic approximation used in astrophysics.
Findings
Massless scalar fields' support extends beyond the light cone in curved space.
Eikonalization does not always produce null geodesics in curved spacetime.
Massive particles follow standard geodesics, unaffected by wave effects.
Abstract
Since particles obey wave equations, in general one is not free to postulate that particles move on the geodesics associated with test particles. Rather, for this to be the case one has to be able to derive such behavior starting from the equations of motion that the particles obey, and to do so one can employ the eikonal approximation. To see what kind of trajectories might occur we explore the domain of support of the propagators associated with the wave equations. For a minimally coupled massless scalar field the domain of support in curved space is shown to not be restricted to the light cone, while for a conformally coupled massless scalar field the curved space domain is only restricted to the light cone if it propagates in a conformal to flat background. Consequently, eikonalization does not in general lead to null geodesics for curved space massless rays even though it does lead…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Geophysics and Gravity Measurements
