Effects of a positive cosmological constant on circular orbits in the Reissner-Nordstroem, Schwarzschild, and Kerr fields

DOI10.1007/BF00764269zbMath0472.53067MaRDI QIDQ1157803

Robert J. Howes

Publication date: 1981

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

zbMATH Keywords

Einstein's field equationscosmological constantstability of circular orbitsaxial symmetric fields

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Applications of global differential geometry to the sciences (53C80)

Related Items (5)

Newtonian analogue of force and motion of a free particle in the gravitational field of Kerr-De Sitter space-time ⋮ The structure of the extreme Schwarzschild-de Sitter space-time ⋮ On some solutions of Maxwell’s equations in a Schwarzschild–de Sitter black hole ⋮ Geodesic portrait of de Sitter-Schwarzschild space-time ⋮ Circular orbits in stationary axisymmetric spacetimes

Cites Work

• The gravity field of a particle

This page was built for publication: Effects of a positive cosmological constant on circular orbits in the Reissner-Nordstroem, Schwarzschild, and Kerr fields