On the latitudinal and radial motion of timelike vortical trajectories in the Kerr metric

Details On the latitudinal and radial motion of timelike vortical trajectories in the Kerr metric On the latitudinal and radial motion of timelike vortical trajectories in the Kerr metric

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984gregr..16..541l&link_type=abstract

General Relativity and Gravitation (ISSN 0001-7701), vol. 16, June 1984, p. 541-549. Research supported by the Natural Sciences

Astronomy and Astrophysics

Astrophysics

2

Astrophysics, Energetic Particles, Equations Of Motion, Particle Trajectories, Space-Time Functions, Conics, Geodesic Lines, Radial Velocity, Trajectory Analysis, Vortices

Scientific paper

The time-like vortical geodesics of the Kerr metric for the trajectories
of escaping high-energy particles is numerically integrated in the
r-theta subspace of the Boyer-Lindquist coordinates. It is found that
under physically reasonable conditions, the trajectories are essentially
conical in the sense of constant theta.

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