The Relativistic Geoid: Gravity Potential and Relativistic Effects

TL;DR

This paper develops a relativistic framework for defining the Earth's geoid within Einstein's General Relativity, enabling high-precision height referencing that accounts for relativistic effects.

Contribution

It introduces a relativistic gravity potential and geoid based on isochronometric surfaces, extending classical geodesy into the relativistic regime with explicit solutions and comparisons.

Findings

Relativistic geoid differs from Newtonian by millimeter-level corrections.

Framework recovers classical results in the appropriate limit.

Explicit solutions for vacuum and post-Newtonian models are provided.

Abstract

The Earth's geoid is one of the most essential and fundamental concepts to provide a gravity field-related height reference in geodesy and associated sciences. To keep up with the ever-increasing experimental capabilities and to consistently interpret high-precision measurements without any doubt, a relativistic treatment of geodetic notions (including the geoid) within Einstein's theory of General Relativity is inevitable. Building on the theoretical construction of isochronometric surfaces and the so-called redshift potential for clock comparison, we define a relativistic gravity potential as a generalization of (post-)Newtonian notions. This potential exists in any stationary configuration with rigidly co-rotating observers, and it is the same as realized by local plumb lines. In a second step, we employ the gravity potential to define the relativistic geoid in direct analogy to the Newtonian understanding. In the respective limit, the framework allows to recover well-known (post-) Newtonian results. For a better illustration and proper interpretation of the general relativistic gravity potential and geoid, some particular examples are considered. Explicit results are derived for exact vacuum solutions to Einstein's field equation as well as a parametrized post-Newtonian model. Comparing the Earth's Newtonian geoid to its relativistic generalization is a very subtle problem, but of high interest. An isometric embedding into Euclidean three-dimensional space is an appropriate solution and allows a genuinely intrinsic comparison. With this method, the leading-order differences are determined, which are at the mm-level.