activity
20042026
most citedA causal Schwarzschild-de Sitter interior solution by gravitational decoupling

130 citations · 400 across the 12 of their papers we have counts for

collaborators

12 papers

gr-qc2026

Non-Schwarzschild black holes sourced by scalar-vector fields

Manuel Gonzalez-Espinoza, Y. Gómez-Leyton, Z. Stuchlik +1

In this work, we construct a static and spherically symmetric black hole solution sourced by a nonlinear scalar-vector sector within the framework of the Minimal Geometric Deformat…

gr-qc2023★ 7 cited

Carter-constant induced mechanism for generation of anisotropic kinetic equilibria in collisionless N-body systems

Claudio Cremaschini, Zdeněk Stuchlík

A new intrinsically-relativistic kinetic mechanism for generation of non-isotropic relativistic kinetic equilibria in collisionless N-body systems is pointed out. The theory is dev…

gr-qc2022

Adiabatic theory in Kerr spacetimes

Kuantay Boshkayev, Gulmira Nurbakyt, Hernando Quevedo +7

We present the main aspects of the adiabatic theory and show that it can be used to study the motion of test particles in general relativity. The theory is based upon the use of ve…

gr-qc2019★ 130 cited

A causal Schwarzschild-de Sitter interior solution by gravitational decoupling

L. Gabbanelli, J. Ovalle, A. Sotomayor +2

We employ the minimal geometric deformation approach to gravitational decoupling (MGD- decoupling) in order to build an exact anisotropic version of the Schwarzschild interior solu…

gr-qc2018★ 3 cited

Exact solution for a black hole embedded in a nonstatic dust-filled universe

Elena Kopteva, Pavlina Jaluvkova, Irina Bormotova +1

An exact solution of the Lemaître--Tolman--Bondi class is investigated as a possible model of the Schwarzschild-like black hole embedded in a non-static dust-filled universe for th…

gr-qc2017★ 48 cited

Scalar perturbations of nonsingular nonrotating black holes in conformal gravity

Bobir Toshmatov, Cosimo Bambi, Bobomurat Ahmedov +2

We study scalar and electromagnetic perturbations of a family of nonsingular nonrotating black hole spacetimes that are solutions in a large class of conformally invariant theories…

gr-qc2016

The generalized Lemaitre-Tolman-Bondi solutions with nonzero pressure in modeling the cosmological black holes

E. Kopteva, P. Jaluvkova, Z. Stuchlik

In this work we have obtained the set of new exact solutions of the Einstein equations that generalize the known Lemaitre-Tolman-Bondi solution for the certain case of nonzero pres…

gr-qc2016★ 92 cited

General relativistic polytropes with a repulsive cosmological constant

Zdeněk Stuchlík, Stanislav Hledík, Jan Novotný

Spherically symmetric equilibrium configurations of perfect fluid obeying a polytropic equation of state are studied in spacetimes with a repulsive cosmological constant. The confi…

gr-qc2016★ 52 cited

Efficiency of the Keplerian accretion in the Braneworld Kerr--Newman Spacetimes and mining instability of some naked singularity spacetimes

Martin Blaschke, Zdeněk Stuchlík

We show that the~braneworld rotating Kerr--Newman black hole and naked singularity spacetimes with both positive and negative braneworld tidal charge parameter can be separated int…

gr-qc2016★ 2 cited

The model of the black hole enclosed in dust. The flat space case

Pavlina Jaluvkova, Elena Kopteva, Zdenek Stuchlik

In this work the model is constructed to describe the black hole enclosed in the dust cosmological background in case of zero spatial curvature. This model is based on our exact so…

gr-qc2015★ 5 cited

Shadow of the rotating black hole with quintessential energy in the presence of the plasma

Ahmadjon Abdujabbarov, Bobir Toshmatov, Zdeněk Stuchlík +1

We study the shadow of the rotating black hole with quintessential energy i) in vacuum and ii) in the presence of plasma with radial power-law density. For vacuum case the quintess…

gr-qc2004★ 61 cited

The Aschenbach effect: unexpected topology changes in motion of particles and fluids orbiting rapidly rotating Kerr black holes

Z. Stuchlik, P. Slany, G. Torok +1

Newton's theory predicts that the velocity of free test particles on circular orbits around a spherical gravity center is a decreasing function of the orbital radius , $dV/d…