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相关论文: About Bianchi I with time varying constants

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In this work, we study some physical aspects of unitary evolution of Bianchi-I model. In particular, we study the behavior of the volume and the scale factor as a function of time for the Bianchi-I universe with ultra-relativistic fluid…

广义相对论与量子宇宙学 · 物理学 2016-01-28 Sridip Pal

A method of solving perfect fluid Einstein equations with two commuting spacelike Killing vectors is presented. Given a spacelike 2-dimensional surface in the 3-dimensional nonphysical Minkowski space the field equations reduce to a single…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Adam Szereszewski , Jacek Tafel

We provide a new class of exact solutions for the interior in (2 + 1) dimensional spacetime. The solutions obtained for the perfect fluid model both with and without cosmological constant ($\Lambda$) are found to be regular and singularity…

广义相对论与量子宇宙学 · 物理学 2014-05-02 Farook Rahaman , Piyali Bhar , Ritabrata Biswas , A. A. Usmani

Self-consistent system of spinor, scalar and BI gravitational fields is considered. Exact solutions to the field equations in terms of volume scale of the BI metric are obtained. Einstein field equations in account of the cosmological…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Bijan Saha , Todor Boyadjiev

Lagrangian formulation for perfect fluid equations which hold invariant under the $\ell$-conformal Galilei group with half-integer $\ell$ is proposed. It is based on a Clebsch-type parametrization and reproduces Lagrangian description of…

高能物理 - 理论 · 物理学 2025-12-02 Timofei Snegirev

We derived equations of motion corresponding to Bianchi-I cosmological models in the Lovelock gravity. Equations derived in the general case, without any specific ansatz for any number of spatial dimensions and any order of the Lovelock…

广义相对论与量子宇宙学 · 物理学 2010-01-22 S. A. Pavluchenko

The locally rotationally symmetric tilted perfect fluid Bianchi type V cosmological model provides examples of future geodesically complete spacetimes that admit a `kinematic singularity' at which the fluid congruence is inextendible but…

广义相对论与量子宇宙学 · 物理学 2009-10-06 A. A. Coley , S. Hervik , W. C. Lim , M. A. H. MacCallum

An anisotropic Bianchi type I cosmological model with power-law scalar-field potentials of the form $V(\psi_1,\psi_2)=V_1\psi_1^{\pm\lambda_1}+V_2\psi_2^{\pm\lambda_2}$ is studied within a generalized S\'aez--Ballester--K-essence-like…

广义相对论与量子宇宙学 · 物理学 2026-04-14 J. Socorro , A. Gil-Ocaranza , Juan Luis Pérez

We examine the behaviour of homogeneous, anisotropic space-times, specifically the locally rotationally symmetric Bianchi types $I$ and $VII_o$ in the presence of anisotropic matter. By finding an appropriate constant of the motion, and…

广义相对论与量子宇宙学 · 物理学 2016-04-29 David Sloan

According to standard cosmology, the universe is homogeneous and isotropic at large scales. However, some anisotropies can be observed at the local scale in the universe through various ways. Here we have studied the Bianchi type I model…

广义相对论与量子宇宙学 · 物理学 2022-09-12 Pranjal Sarmah , Umananda Dev Goswami

Suppose $G$ is a compact Lie group, $H$ is a closed subgroup of $G$, and the homogeneous space $G/H$ is connected. The paper investigates the Ricci flow on a manifold $M$ diffeomorphic to $[0,1]\times G/H$. First, we prove a short-time…

偏微分方程分析 · 数学 2017-10-10 Artem Pulemotov

We report some new exact instantons in general relativity. These solutions are K\"ahler and fall into the symmetry classes of Bianchi types VI0 and VII0, with matter content of a stiff fluid. The qualitative behaviour of the solutions is…

广义相对论与量子宇宙学 · 物理学 2009-10-31 J. D. Barrow , Y. Gaspar , P. M. Saffin

We investigate the set of spacetime general coordinate transformations (G.C.T.) which leave the line element of a generic Bianchi Type Geometry, quasi-form invariant; i.e. preserve manifest spatial Homogeneity. We find that these G.C.T.'s,…

广义相对论与量子宇宙学 · 物理学 2009-10-09 T. Christodoulakis , G. Kofinas , E. Korfiatis , G. O. Papadopoulos , A. Paschos

Bianchi type V matter filled universe with varying lambda in general relativity are investigated by using the law of variation for the generalized mean Hubble parameter. This yields the constant value of deceleration parameter and generates…

广义相对论与量子宇宙学 · 物理学 2013-01-15 Anil Kumar Yadav

In our previous article [Rad16], we investigated the asymptotic behaviour of orthogonal Bianchi class B perfect fluids close to the initial singularity and proved the Strong Cosmic Censorship conjecture in this setting. In several of the…

广义相对论与量子宇宙学 · 物理学 2017-12-13 Katharina Radermacher

A mathematical model for description of the viscous fingering induced by a chemical reaction is under study. This complicated five-component model is reduced to a three-component diffusive Lotka-Volterra system with convection by…

数学物理 · 物理学 2025-12-19 Roman Cherniha , Vasyl' Davydovych

In this paper, we explore an axially symmetric Bianchi type-I model of the universe with bulk viscous fluid as a source of gravitational field under the framework of Einstein's field equations by assuming barotropic bulk viscous pressure as…

广义相对论与量子宇宙学 · 物理学 2025-04-29 G. K. Goswami , Anirudh Pradhan , Vipin Chandra Dubey

We investigate the evolution of anisotropies in Bianchi I spacetimes within the framework of the 4D Einstein-Gauss-Bonnet scalar field theory. The field equations are formulated using dimensionless variables, and the asymptotic dynamics are…

广义相对论与量子宇宙学 · 物理学 2026-01-06 Alex Giacomini , Chevara Hansraj , Genly Leon , Andronikos Paliathanasis

In this paper we consider the Einstein-Vlasov system with Bianchi VII$_0$ symmetry. Under the assumption of small data we show that self-similarity breaking occurs for reflection symmetric solutions. This generalizes the previous work…

广义相对论与量子宇宙学 · 物理学 2024-06-21 Ho Lee , Ernesto Nungesser

The general form of the anisotropy parameter of the expansion for Bianchi type-III metric is obtained in the presence of a single diagonal imperfect fluid with a dynamically anisotropic equation of state parameter and a dynamical energy…

广义相对论与量子宇宙学 · 物理学 2014-11-20 Ozgur Akarsu , Can B. Kilinc