The Newtonian forces in the Kerr geometry

Details The Newtonian forces in the Kerr geometry The Newtonian forces in the Kerr geometry

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990japa...11...29c&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 11, March 1990, p. 29-35.

Physics

Optics

5

Accretion Disks, Black Holes (Astronomy), Geometrical Optics, Kerr Magnetooptical Effect, Stellar Rotation, Angular Momentum, Centrifugal Force, Coriolis Effect, Gravitational Effects, Rotary Stability

Scientific paper

The properties of the Newtonian forces acting on a test particle in the field of the Kerr black hole geometry are studied. It is shown that the centrifugal force and the Coriolis force reverse signs at several different locations. The possible relevance of such reversals is noted, particularly in the study of the stability properties of the compact rotating stars and the accretion disks in hydrostatic equilibria.

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