Abstract
We discuss various aspects of the post-Newtonian approximation in general relativity. After presenting the foundation based on the Newtonian limit, we use the (3+1) formalism to formulate the post-Newtonian approximation for the perfect fluid. As an application we show the method for constructing the equilibrium configuration of non-axisymmetric uniformly rotating fluid. We also discuss the gravitational waves including tail from post-Newtonian systems.
Original language | English |
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Pages (from-to) | 123-181 |
Number of pages | 59 |
Journal | Progress of Theoretical Physics Supplement |
Issue number | 128 |
DOIs | |
Publication status | Published - 1997 |
Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)