Geodesics in black hole space-times

DOI10.1007/BF00756902zbMath0433.53052MaRDI QIDQ1139300

N. A. Sharp

Publication date: 1979

Published in: General Relativity and Gravitation (Search for Journal in Brave)

zbMATH Keywords

geodesicsequations of motionblack holesKerr-Newman geometry

Mathematics Subject Classification ID

Applications of global differential geometry to the sciences (53C80) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Geodesics in global differential geometry (53C22) Equations of motion in general relativity and gravitational theory (83C10)

Related Items

Particle dynamics around weakly magnetized Reissner-Nordström black hole, Revisiting timelike and null geodesics in the Schwarzschild spacetime: general expressions in terms of Weierstrass elliptic functions, Polar orbits in the Kerr space-time, Second order Kerr deflection, Geodesics on a Kerr-Newman-(anti-)de Sitter instanton, Photon boomerang in a nearly extreme Kerr metric, Region of magnetic dominance near a rotating black hole, Orbital dynamics of the charged particle In the gravitational field of Kehagias-Sfetsos black hole In Horova-Lifshitz gravity In presence of external magnetic field, Spherical photon orbits around a Kerr black hole, Phase-plane analysis of periastron procession about a Reissner-Nordström black hole, Gravitational lensing from a spacetime perspective, Analytical Solutions for Geodesic Equation in Black Hole Spacetimes, Motion of test particles in a regular black hole space–time, Theoretical aspects of relativistic spectral features, Orbits through the ergosphere of a Kerr black hole, Dynamics and center of mass energy of colliding particles around black hole in f(R) gravity

Cites Work

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• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• On Energy Stored in Linear Viscoelastic Solids
• Maximal Analytic Extension of the Kerr Metric
• Global Structure of the Kerr Family of Gravitational Fields
• Observable Properties of Large Relativistic Masses