Post-Newtonian Equations of Motion in Flat Cosmological Models

Details Post-Newtonian Equations of Motion in Flat Cosmological Models Post-Newtonian Equations of Motion in Flat Cosmological Models

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pthph..85.1041t&link_type=abstract

Progress of Theoretical Physics, Vol. 85, No. 5, pp. 1041-1047

Physics

17

Scientific paper

The post-Newtonian equations of motion for particles in an expanding universe are derived in spatially flat models with cosmological constant. This system of equations is an extended version of the previous one which was derived in the Einstein-de Sitter model. The applicability condition is also examined and some errors found in the previous expressions are indicated and corrected.

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