MY Khlopov - Research in Astronomy and Astrophysics, 2010 - iopscience.iop.org
Primordial black holes (PBHs) are a profound signature of primordial cosmological structures and provide a theoretical tool to study nontrivial physics of the early Universe. The …
M Garbiso, M Kaminski - Journal of High Energy Physics, 2020 - Springer
A bstract We find hydrodynamic behavior in large simply spinning five-dimensional Anti-de Sitter black holes. These are dual to spinning quantum fluids through the AdS/CFT …
We study scalar, electromagnetic, and gravitational test fields in the Hayward, Bardeen, and Ayón-Beato-García regular black hole spacetimes and demonstrate that the test fields are …
T Takahashi, J Soda - Progress of Theoretical Physics, 2010 - academic.oup.com
In this paper, we derive the master equations for gravitational perturbations of vector and scalar type for static vacuum Lovelock black holes. Together with our previous work on the …
C Charmousis, B Goutéraux, J Soda - Physical Review D—Particles, Fields …, 2009 - APS
We find and analyze solutions of Einstein's equations in arbitrary dimensions and in the presence of a scalar field with a Liouville potential coupled to a Maxwell field. We consider …
RA Konoplya, A Zhidenko - Physical Review D—Particles, Fields, Gravitation …, 2008 - APS
We investigate stability of the D-dimensional Reissner-Nordström-anti-de Sitter metrics as solutions of the Einstein-Maxwell equations. We have shown that asymptotically anti-de …
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 …
T Takahashi, J Soda - Progress of theoretical physics, 2010 - academic.oup.com
We study the stability of static black holes in Lovelock theory which is a natural higher dimensional generalization of Einstein theory. We show that Lovelock black holes are stable …
We study the stability of AdS black holes rotating in a single two-plane for tensor-type gravitational perturbations in D> 6 space-time dimensions. First, by an analytic method, we …