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Arbitrarily long-lived quasinormal modes in a wormhole background of massive fields for a number of black-hole backgrounds at some discrete values of mass of the field. Here

General parametrization of black holes: The only parameters that matterThe general parametrization of a black-hole spacetime in arbitrary metric theories of gravity

Einstein-scalar-Gauss-Bonnet black holes: Analytical approximation for the metric and applications to calculations of shadows of the continued-faction expansion in terms of a compact coordinate in order to obtain an analytical approximation

Shadows of parametrized axially symmetric black holes allowing for separation of variables on a few deformation parameters only. We analyze the influence of these parameters on the black

Analytical representation for metrics of scalarized Einstein-Maxwell black holes and their shadows

Instabilities of wormholes and regular black holes supported by a phantom scalar fieldWe test the stability of various wormholes and black holes supported by a scalar field with a

Echoes of compact objects: New physics near the surface and matter at a distanceIt is well known that a hypothetical compact object that looks like an Einsteinian (Schwarzschild

On the stability of scalar-vacuum space-timesWe study the stability of static, spherically symmetric solutions to the Einstein equations with a

No stable wormholes in Einstein-dilaton-Gauss-Bonnet theory. The exponential growth appears in the time domain after a long period of damped oscillations, in the same way

Black holes in the four-dimensional Einstein-Lovelock gravityA (3+1)-dimensional Einstein-Gauss-Bonnet theory of gravity has been recently formulated by Glavan

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