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    The Motion of Test Particles in Black-Hole Backgrounds with Non-Zero Cosmological Constant

    Zdeněk Stuchlík · Červen 01, 1983 · Fyzika · 0 comments
    0

    Publication date: Jun 1983

    Abstract:
    Due to the present indications of the existence of a non-zero
    cosmological constant, some aspects of the influence of a Lambda not
    equal to zero on the character of test-particle motion in black-hole
    backgrounds are discussed. Equations of motion of electrically charged
    particles and magnetic monopoles are written in the most general Kerr-
    Newman-de Sitter dyon background. For the Kerr-de Sitter spacetime, the
    latitudinal motion is examined in detail by using the ‚Chinese boxes‘
    technique. The radial motion in the Schwarzschild-de Sitter background
    is considered with attention devoted to the existence and stability of
    circular orbits and to the properties of purely radial trajectories.
    Finally, the possibility of constructing an Einstein-Strauss-de Sitter
    model of the Universe (i.e. a model of Schwarzschild-de Sitter
    condensations in the Friedman Universe with a non-zero Lambda-term) is
    discussed.

    Authors:
    Stuchlik, Z.;

    https://ui.adsabs.harvard.edu/abs/1983BAICz..34..129S

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