activity
20032009
most citedStability and quasinormal modes of the massive scalar field around Kerr black holes

145 citations · 1.3k across the 17 of their papers we have counts for

collaborators
Showing hep-thShow all

18 papers · 1 filter

hep-th2009138 cited

Towards constraining of the Horava-Lifshitz gravities

R. A. Konoplya

Recently a renormalizable model of gravity has been proposed, which might be a UV completion of General Relativity (GR) or its infra-red modification, probably with a strongly coup…

hep-th200972 cited

Gravitational instability of simply rotating AdS black holes in higher dimensions

Hideo Kodama, R. A. Konoplya, A. Zhidenko

We study the stability of AdS black hole holes rotating in a single two plane for tensor-type gravitational perturbations in space-time dimensions. First, by an analytic me…

hep-th200893 cited

Stability of higher dimensional Reissner-Nordstrom-anti-de Sitter black holes

R. A. Konoplya, A. Zhidenko

We investigate stability of the D-dimensional Reissner-Nordstrom-anti-de-Sitter metrics as solutions of the Einstein-Maxwell equations. We have shown that asymptotically anti-de Si…

hep-th2008111 cited

Instability of higher dimensional charged black holes in the de-Sitter world

R. A. Konoplya, A. Zhidenko

We have shown that higher dimensional Reissner-Nordström-de Sitter black holes are gravitationally unstable for large values of the electric charge and cosmological constant in $D…

hep-th200844 cited

Looking at the Gregory-Laflamme instability through quasi-normal modes

R. A. Konoplya, Keiju Murata, Jiro Soda +1

We study evolution of gravitational perturbations of black strings. It is well known that for all wavenumber less than some threshold value, the black string is unstable against sc…

hep-th2008106 cited

Evolution of perturbations of squashed Kaluza-Klein black holes: escape from instability

Hideki Ishihara, Masashi Kimura, Roman A. Konoplya +3

The squashed Kaluza-Klien (KK) black holes differ from the Schwarzschild black holes with asymptotic flatness or the black strings even at energies for which the KK modes are not e…