A quasi-stationary approximation for the equations of motion of a black hole

Details A quasi-stationary approximation for the equations of motion of a black hole A quasi-stationary approximation for the equations of motion of a black hole

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980fiz....23...21z&link_type=abstract

Fizika, vol. 23, Nov. 1980, p. 21-26. In Russian.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Black Holes (Astronomy), Equations Of Motion, Quasi-Steady States, Differential Equations, Integral Equations, Relativity, Space-Time Functions

Scientific paper

The motion of a black hole under external influences is considered from the point of view of a distant observer. Zerilli equations are used to detect the hole's displacement and the structure of the metric in the presence of other gravitational bodies. It is shown that in a region where the curvature of space is slight, the contribution of the field of a rapidly moving black hole coincides in form with the field of an ordinary body. The motion of a black hole in the quasistationary approximation is governed by laws of Newtonian dynamics.

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