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
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
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