A universal tool for determining the time delay and the frequency shift of light: Synge's world function
Pierre Teyssandier, Christophe Le Poncin-Lafitte, Bernard Linet

TL;DR
This paper introduces a universal method to calculate light's time delay and frequency shift using Synge's world function, avoiding geodesic integration, with explicit formulas for gravitational effects up to order 1/c^4.
Contribution
It derives the Synge's world function up to order 1/c^3 within PPN formalism, enabling direct calculations of light effects without solving geodesic equations.
Findings
Explicit formulas for mass, quadrupole, and angular momentum contributions.
Quadrupole-induced frequency shift of 10^-16 for Earth's parameters.
Method applicable to stationary, axisymmetric gravitational fields.
Abstract
In almost all of the studies devoted to the time delay and the frequency shift of light, the calculations are based on the integration of the null geodesic equations. However, the above-mentioned effects can be calculated without integrating the geodesic equations if one is able to determine the bifunction giving half the squared geodesic distance between two points and (this bifunction may be called Synge's world function). In this lecture, is determined up to the order within the framework of the PPN formalism. The case of a stationary gravitational field generated by an isolated, slowly rotating axisymmetric body is studied in detail. The calculation of the time delay and the frequency shift is carried out up to the order . Explicit formulae are obtained for the contributions of the mass, of the quadrupole moment and of…
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