activity
20062026
most citedAnisotropic cosmological models in Horndeski gravity

28 citations · 97 across the 12 of their papers we have counts for

collaborators

12 papers

gr-qc2026

Models of exponential and power-law acceleration of the Universe in Horndeski theory without ghosts and Laplace instabilities

Ruslan K. Muharlyamov, Tatiana N. Pankratyeva, Shehabaldeen O. A. Bashir

We present a designer method for flat Friedman-Robertson-Walker space-times within the framework of Horndeski's scalar-tensor theory. As a result, one can find subclasses of Hornde…

gr-qc2024★ 1 cited

Exact cosmological solutions with magnetic field in the theory of gravity with non-minimal kinetic coupling

Ruslan K. Muharlyamov, Tatiana N. Pankratyeva, Shehabaldeen O. A. Bashir

We investigate anisotropic and homogeneous cosmological models in the scalar-tensor theory of gravity with non-minimal kinetic coupling of a scalar field to the curvature given by…

gr-qc2024★ 3 cited

Magnetic Bianchi-I cosmology in the Horndeski theory

Ruslan K. Muharlyamov, Tatiana N. Pankratyeva, Shehabaldeen O. A. Bashir

We study the evolution of Bianchi-I space-times within the framework of the Horndeski theory with . The space-times are filled a global unidirectional electroma…

gr-qc2021★ 6 cited

Reconstruction in the Horndeski theory within the scope of the Bianchi I cosmology

Ruslan K. Muharlyamov, Tatiana N. Pankratyeva

In the previous article Eur. Phys. J. Plus 136, 590 (2021) (arXiv: 2110.15396) we have proposed a reconstruction method for the kinetic gravity braiding theory in the framework of…

gr-qc2021★ 9 cited

Reconstruction method in the kinetic gravity braiding theory with shift-symmetric

Ruslan K. Muharlyamov, Tatiana N. Pankratyeva

We present a reconstruction method for flat Friedman-Robertson-Walker (FRW) spacetime in a subclass of Horndeski theory -- specifically shiftsymmetric, the kinetic gravity braiding…

gr-qc2021★ 4 cited

The nonlinear anisotropic model of the Universe with the linear potential

Ruslan K. Muharlyamov, Tatiana N. Pankratyeva

In the Bianchi I cosmology some subclasses of the Horndeski theory allow for the non-standard anisotropy behavior. For example, the anisotropy is damped near the initial singularit…

gr-qc2021★ 28 cited

Anisotropic cosmological models in Horndeski gravity

Rafkat Galeev, Ruslan Muharlyamov, Alexei A. Starobinsky +2

It was found recently that the anisotropies in the homogeneous Bianchi I cosmology considered within the context of a specific Horndeski theory are damped near the initial singular…

gr-qc2014★ 14 cited

Axion-induced oscillations of cooperative electric field in a cosmic magneto-active plasma

Alexander B. Balakin, Ruslan K. Muharlyamov, Alexei E. Zayats

We consider one cosmological application of an axionic extension of the Maxwell-Vlasov theory, which describes axionically induced oscillatory regime in the state of global magneti…

gr-qc2013★ 14 cited

Electromagnetic waves in an axion-active relativistic plasma non-minimally coupled to gravity

Alexander B. Balakin, Ruslan K. Muharlyamov, Alexei E. Zayats

We consider cosmological applications of a new self-consistent system of equations, accounting for a nonminimal coupling of the gravitational, electromagnetic and pseudoscalar (axi…

gr-qc2013★ 15 cited

Nonminimal Einstein-Maxwell-Vlasov-axion model

Alexander B. Balakin, Ruslan K. Muharlyamov, Alexei E. Zayats

We establish a new self-consistent system of equations accounting for a nonminimal coupling of the cooperative gravitational, electromagnetic and pseudoscalar (axion) fields in a m…

gr-qc2008★ 3 cited

Non-minimal electrodynamics and resonance interactions in relativistic plasma

A. B. Balakin, R. K. Muharlyamov

A three-parameter toy-model, which describes a non-minimal coupling of gravity field with electromagnetic field of a relativistic two-component electrically neutral plasma, is disc…

gr-qc2006

Local spherically symmetric perturbations of spatially flat Friedmann models

A. A. Popov, R. K. Muharlyamov

The spherically symmetric perturbations in the spatially flat Friedman models are considered. It is assumed that the Friedmannian density and pressure are related through a linear…