Testing a theory of gravity in celestial mechanics: a new method and its first results for a scalar theory

TL;DR

This paper introduces a rigorous post-Newtonian approximation method for weak gravitational fields, applied to test a scalar theory of gravity, revealing the influence of internal structure on celestial motion.

Contribution

It presents a new PNA method based on a one-parameter family of systems, differing from standard PNA, and applies it to test a scalar gravity theory in the solar system.

Findings

The new method predicts internal structure influences on motion.

Comparison with standard PNA shows differences in celestial predictions.

First results demonstrate the method's applicability to scalar gravity theories.

Abstract

A new method of post-Newtonian approximation (PNA) for weak gravitational fields is presented together with its application to test an alternative, scalar theory of gravitation. The new method consists in defining a one-parameter family of systems, by applying a Newtonian similarity transformation to the initial data that defines the system of interest. This method is rigorous. Its difference with the standard PNA is emphasized. In particular, the new method predicts that the internal structure of the bodies does have an influence on the motion of the mass centers. The translational equations of motion obtained with this method in the scalar theory are adjusted in the solar system, and compared with an ephemeris based on the standard PNA of GR.