Comparison between two methods of post-Newtonian expansion for the motion in a weak Schwarzschild field
Mayeul Arminjon

TL;DR
This paper compares the asymptotic and standard post-Newtonian methods for modeling a test particle's motion in a weak Schwarzschild field, finding they are equivalent with proper reinitialization, and discusses their differences and applications.
Contribution
It introduces a detailed comparison between the asymptotic and standard PN expansion methods in weak gravitational fields, highlighting their equivalence and practical considerations.
Findings
Asymptotic and standard PN methods produce similar results when reinitialized properly.
The deviation between methods grows quadratically with time if not reinitialized.
Both methods are valid, but the asymptotic approach is more natural in general cases.
Abstract
The asymptotic method of post-Newtonian (PN) expansion for weak gravitational fields, recently developed, is compared with the standard method of PN expansion, in the particular case of a massive test particle moving along a geodesic line of a weak Schwarzschild field. First, the expression of the active mass in Schwarzschild's solution is given for a barotropic perfect fluid, both for general relativity (GR) and for an alternative, scalar theory. The principle of the asymptotic method is then recalled and the PN expansion of the active mass is derived. The PN correction to the active mass is made of the Newtonian elastic energy, augmented, for the scalar theory, by a term due to the self-reinforcement of the gravitational field. Third, two equations, both correct to first order, are derived for the geodesic motion of a mass particle: a "standard" one and an "asymptotic" one. Finally,…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Relativity and Gravitational Theory
