Astronomical tests in a Kerr field

Details Astronomical tests in a Kerr field Astronomical tests in a Kerr field

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.123...21k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 123, no. 1, June 1986, p. 21-29.

Statistics

Computation

2

Computational Astrophysics, Stellar Magnetic Fields, Stellar Rotation, Integral Equations, Kerr Effects, Light Scattering, Red Shift, Schwarzschild Metric

Scientific paper

The astronomical effects that occur in the equatorial plane of a stellar object due to rotation according to Kerr theory are calculated in the lowest order of approximation. The four possible tests known in Schwarzschild theory are considered, and only the advance of perihelion and the bending of a light beam show deviations in the equatorial plane of an astrophysical object according to Kerr theory.

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