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  • Некоторые метрики заблокированы вашими 
    Тип записи:Публикация,
    Gravitational field of slightly deformed naked singularities
    (Springer Science+Business Media, 2022-04-01) ;
    Hernando Quevedo
    ;
    Medeu Abishev
    ;
    Aray Muratkhan
    Abstract We derive a particular approximate solution of Einstein equations, describing the gravitational field of a mass distribution that slightly deviates from spherical symmetry. The deviation is described by means of a quadrupole parameter that is responsible for the appearance of a curvature singularity, which is not covered by a horizon. We investigate the motion of test particles in the gravitational field of this naked singularity and show that the quadrupole parameter affects the properties of Schwarzschild trajectories. By investigating radial geodesics, we find that no effects of repulsive gravity are present. We interpreted this result as indicating that repulsive gravity is non-linear effect.
    Цитирования (OpenAlex) 12Цитирования (OpenCitations) 9
  • Некоторые метрики заблокированы вашими 
    Тип записи:Публикация,
    Black holes with multiple horizons without mass inflation
    (Springer Science+Business Media, 2026-05-06)
    Changjun Gao
    ;
    Abstract Mass inflation is a phenomenon occurring in the vicinity of the inner horizon in a spacetime with two horizons. It is shown that the mass of initially small perturbations grows exponentially as they approach the inner horizon. This implies that the inner horizon of a black hole is unstable under perturbations. Since mass inflation is determined by the surface gravities of the inner horizons, Carballo-Rubio et al. showed that if one makes the surface gravities of the inner horizons vanish, then the exponential growth associated with mass inflation is not present. Based on this conclusion, we look for the black hole solutions of multiple horizons in the presence of a nonlinear Maxwell field. We then make the inner horizons coincide with each other such that the surface gravities of all inner horizons vanish. In this way, black holes with multiple horizons without mass inflation are constructed.
    Цитирования (OpenAlex) 2