Computer Science – Performance
Scientific paper
Sep 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982gregr..14..793s&link_type=abstract
General Relativity and Gravitation, vol. 14, Sept. 1982, p. 793-805. Research supported by the British Council and Consejo Naci
Computer Science
Performance
8
Formalism, Gravitational Fields, Relativity, Solar System, Approximation, Equations Of Motion, Newton Theory, Particle Motion, Particle Trajectories, Performance Tests
Scientific paper
An extension of the parametrized post-Newtonian (PPN) formalism to third order in the expansion parameter m/r is used to derive analytical expressions accurate to the same order for the motion of test particles and photons in the presence of the gravitational field of the sun represented by a static, isotropic metric. The consequences of including higher-order terms are discussed in relation to the so-called classical gravitational tests for the case of general relativity theory. Present observational or experimental data are not accurate enough to detect variations due to the inclusion of higher-order terms but a planned solar probe experiment may provide information that would make such detection possible.
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