The General Method for Fixing the Gauges of Relativistic Astronomical Reference Systems

@article{Tao2006TheGM,
  title={The General Method for Fixing the Gauges of Relativistic Astronomical Reference Systems},
  author={Jin-he Tao},
  journal={Astrophysics and Space Science},
  year={2006},
  volume={302},
  pages={93-98}
}
  • Jin-he Tao
  • Published 29 April 2006
  • Physics
  • Astrophysics and Space Science
This article applies a new scheme of the first post-Newtonian theory (Damour et al., 1991–1994) to the problem of gauge in relativistic reference systems. Choosing and fixing gauge are necessary when the precision of time measurement and application needs to reach the 2PN level (10−16 or better). We present a general method for fixing the gauges of both the global and local coordinate systems, and for determining the expressions of gravitational potentials and coordinate transformations. The… 
Astronomical relativistic reference systems with multipolar expansion: the global one
With the rapid development of techniques for astronomical observations, the precision of measurements has been significantly increasing. Theories describing astronomical relativistic reference

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