Statistics – Computation
Scientific paper
Aug 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.194..159y&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 194, no. 1, p. 159-163.
Statistics
Computation
3
Binary Stars, Gravitational Waves, Pulsars, Relativity, Computational Astrophysics, Stellar Orbits
Scientific paper
The predictions of Einstein's theory of general relativity (GR) with respect to the gravitational radiation of PSR 1913+16 are examined to determine whether they are self-consistent in the context of GR. The GR approximation for gravitational radiation is given and applied to a finite neutral particle system. It is shown that the Einsteinian approximation yields no gravitational radiation, and Newtonian orbits are theorized to be adequate for describing the rate of change of the orbital period of PSR 1913+16.
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