Results 1 to 10 of about 1,949 (157)
Bianchi I metric solutions with nonminimally coupled Einstein–Maxwell gravity theory [PDF]
38 pages, 2 figures, 6 ...
Hossein Ghaffarnejad +1 more
exaly +3 more sources
Bianchi type–I Model with Time Varying Λ and G: The Generalized Solution
In this paper, we have investigated the homogeneous and anisotropic Bianchi type–I cosmological model with a time-varying Newtonian and cosmological constant.
Aha Alfedeel
exaly +2 more sources
Beyond the linear analysis of stability in higher derivative gravity with the Bianchi-I metric [PDF]
11 pages, 11 ...
Ilya Shapiro, Grigori Chapiro
exaly +3 more sources
Curvature properties of a metric connection with totally skew-symmetric torsion are investigated. It is shown that if either the 3-form $T$ is harmonic, $dT=δT=0$ or the curvature of the torsion connection $R\in S^2Λ^2$ then the scalar curvature of a $\nabla$-Einstein manifold is determined by the norm of the torsion up to a constant. It is proved that
Ivanov S
exaly +3 more sources
Killing vector fields of locally rotationally symmetric Bianchi type V spacetime [PDF]
The classification of locally rotationally symmetric Bianchi type V spacetime based on its killing vector fields is presented in this paper using an algebraic method.
Shakeel Ahmad +4 more
doaj +2 more sources
On the Completeness of Some Bianchi Type A and Related Kähler–Einstein Metrics [PDF]
minor ...
Maschler, Gideon, Ream, Robert
openaire +3 more sources
Symmetries of locally rotationally symmetric Bianchi type V spacetime
In this paper, we classify the metric of locally rotationally symmetric Bianchi type V spacetime through its symmetries, including Killing, homothetic and conformal vector fields.
Jamshed Khan +3 more
doaj +1 more source
Scalar field cosmologies with a generalized harmonic potential and a matter fluid with a barotropic Equation of State (EoS) with barotropic index $$\gamma $$ γ for locally rotationally symmetric (LRS) Bianchi III metric and open Friedmann–Lemaître ...
Genly Leon +4 more
doaj +1 more source
Cosmological Solutions of Integrable F(R) Gravity Models with an Additional Scalar Field
We consider F(R) cosmological models with a scalar field. For the R2 model in the spatially flat Friedmann–Lemaître–Robertson–Walker metric, the Ricci scalar R can smoothly change its sign during the evolution if and only if the scalar field is a phantom
Sergey Vernov, Vsevolod Ivanov
doaj +1 more source
Homogeneous and anisotropic universe models with bouncing deceleration parameter in $f(R,T)$ theory
In this study, we have investigated the cloud of string with perfect fluid (CSPF) matter distribution for the homogeneous and anisotropic (Bianchi I, III, and Kantowski-Sachs) universe models in the $f(R,T)$ theory.
Aysel Kızılcık, Can Aktaş
doaj +1 more source

