The intrinsic derivative and centrifugal forces in general relativity: II. Applications to circular orbits in some familiar stationary axisymmetric spacetimes

Details The intrinsic derivative and centrifugal forces in general relativity: II. Applications to circular orbits in some familiar stationary axisymmetric spacetimes The intrinsic derivative and centrifugal forces in general relativity: II. Applications to circular orbits in some familiar stationary axisymmetric spacetimes

2001-06-05

arxiv.org/abs/gr-qc/0106014v1

Int.J.Mod.Phys.D6:143-198,1997

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

59 pages latex 2.09, uses ijmpd.sty macros, pictex, epsf.sty for 10 eps figures; typographical corrections made compared to pu

Scientific paper

10.1142/S021827189700011X

The tools developed in a preceding article for interpreting spacetime geometry in terms of all possible space-plus-time splitting approaches are applied to circular orbits in some familiar stationary axisymmetric spacetimes. This helps give a more intuitive picture of their rotational features including spin precession effects, and puts related work of Abramowicz, de Felice, and others on circular orbits in black hole spacetimes into a more general context.

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