AbstractA detailed numerical stability analysis of the static, spherically symmetric globally regular solutions of the Einstein–Yang–Mills equations with a positive cosmological constant, Λ, is carried out. It is found that the number of unstable modes in the even parity sector is n for solutions with n=1,2 nodes as Λ varies. The solution with n=3 nodes exhibits a rather surprising behaviour in that the number of its unstable modes jumps from 3 to 1 as Λ crosses (from below) a critical value. In particular the topologically 3-sphere type solution with n=3 nodes has only a single unstable mode
AbstractWe explore via linearized perturbation theory the Gregory–Laflamme instability of the black ...
We construct hairy static black holes of higher dimensional general coupling Einstein-Skyrme theorie...
Instability of 6 dimensional Rubakov-Shaposhnikov model is reinvestigated. It is shown that the mode...
AbstractA detailed numerical stability analysis of the static, spherically symmetric globally regula...
We investigate the stability of spherically symmetric, purely magnetic, soliton and black hole solut...
We investigate the stability of spherically symmetric, purely magnetic, soliton and black hole solut...
A (n+ 1) -dimensional gravitational model with Gauss–Bonnet term and a cosmological constant term is...
A (n+ 1) -dimensional gravitational model with Gauss–Bonnet term and a cosmological constant term is...
The equations describing the adiabatic, small radial oscillations of general relativistic stars are ...
We consider steady state solutions of the massive, asymptotically flat, spherically symmetric Einste...
We study the nonlinear evolution of a weakly perturbed anti-de Sitter (AdS) spacetime by solving num...
It is well known that the U(1) Reissner–Nordström black hole is stable within the framework of the E...
AbstractIt is well known that the U(1) Reissner–Nordström black hole is stable within the framework ...
We consider five-dimensional, vacuum Einstein equations with negative cosmological constant within c...
A $$(n+1)$$-dimensional gravitational model with Gauss–Bonnet term and a cosmological constant term ...
AbstractWe explore via linearized perturbation theory the Gregory–Laflamme instability of the black ...
We construct hairy static black holes of higher dimensional general coupling Einstein-Skyrme theorie...
Instability of 6 dimensional Rubakov-Shaposhnikov model is reinvestigated. It is shown that the mode...
AbstractA detailed numerical stability analysis of the static, spherically symmetric globally regula...
We investigate the stability of spherically symmetric, purely magnetic, soliton and black hole solut...
We investigate the stability of spherically symmetric, purely magnetic, soliton and black hole solut...
A (n+ 1) -dimensional gravitational model with Gauss–Bonnet term and a cosmological constant term is...
A (n+ 1) -dimensional gravitational model with Gauss–Bonnet term and a cosmological constant term is...
The equations describing the adiabatic, small radial oscillations of general relativistic stars are ...
We consider steady state solutions of the massive, asymptotically flat, spherically symmetric Einste...
We study the nonlinear evolution of a weakly perturbed anti-de Sitter (AdS) spacetime by solving num...
It is well known that the U(1) Reissner–Nordström black hole is stable within the framework of the E...
AbstractIt is well known that the U(1) Reissner–Nordström black hole is stable within the framework ...
We consider five-dimensional, vacuum Einstein equations with negative cosmological constant within c...
A $$(n+1)$$-dimensional gravitational model with Gauss–Bonnet term and a cosmological constant term ...
AbstractWe explore via linearized perturbation theory the Gregory–Laflamme instability of the black ...
We construct hairy static black holes of higher dimensional general coupling Einstein-Skyrme theorie...
Instability of 6 dimensional Rubakov-Shaposhnikov model is reinvestigated. It is shown that the mode...