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相关论文: An anisotropic Kantowski-Sachs universe with radia…

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We consider the cosmological evolution of a flat anisotropic Universe in $f(T)$ gravity in the presence of a perfect fluid. It is shown that the matter content of the Universe has a significant impact of the nature of a cosmological…

广义相对论与量子宇宙学 · 物理学 2021-06-10 Maria A. Skugoreva , Alexey V. Toporensky

We construct general anisotropic cosmological scenarios governed by an $f(R)$ gravitational sector. Focusing then on Kantowski-Sachs geometries in the case of $R^n$-gravity, and modelling the matter content as a perfect fluid, we perform a…

广义相对论与量子宇宙学 · 物理学 2011-08-19 Genly Leon , Emmanuel N. Saridakis

We investigate a simple inhomogeneous anisotropic cosmology (plane symmetric $G_2$ model) filled with a tilted perfect fluid undergoing velocity diffusion on a scalar field. Considered are two types of fluid: dust and radiation. We solve…

广义相对论与量子宇宙学 · 物理学 2014-11-13 Dmitry Shogin , Sigbjorn Hervik

Following recent considerations of a non-zero value for the vacuum energy density and the realization that a simple Kantowski-Sachs model might fit the classical tests of cosmology, we study the qualitative behavior of three anisotropic and…

天体物理学 · 物理学 2011-04-15 Paulo Aguiar , Paulo Crawford

Following the recent recognition of a positive value for the vacuum energy density and the realization that a simple Kantowski-Sachs model might fit the classical tests of cosmology, we study the qualitative behavior of three anisotropic…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Paulo Aguiar , Paulo Crawford

We present an anisotropic cosmological model based on a new exact solution of Einstein equations. The matter content consists of an anisotropic scalar field minimally coupled to gravity and of two isotropic perfect fluids that represent…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Saulo Carneiro , Guillermo A. Mena Marugan

We construct a model of a universe filled with a perfect fluid with isotropic particle pressure. The anisotropic plane symmetric Kasner spacetime is used as a seed metric and through a conformal mapping a perfect fluid is generated. The…

广义相对论与量子宇宙学 · 物理学 2018-08-29 Sudan Hansraj , Megandhren Govender , Narenee Mewalal

In this work we consider the Kantowski-Sachs (KS) universe in the framework of varying speed of light theory. We present the general solutions of the gravitational field equations with variable speed of light $c(t)$, gravitational coupling…

综合物理 · 物理学 2016-06-27 G. S. Khadekar , Arti Ghogre , Saibal Ray

We consider a cosmological model in which the two major fluid components of the Universe, dark energy and dark matter, flow with distinct four-velocities. This cosmological configuration is equivalent to a single anisotropic fluid,…

广义相对论与量子宇宙学 · 物理学 2013-07-24 Tiberiu Harko , Francisco S. N. Lobo

The cosmological principle asserts that on sufficiently large scales the Universe is homogeneous and isotropic on spatial slices. To deviate from this principle requires a departure from the FLRW ansatz. In this paper we analyze the…

宇宙学与河外天体物理 · 物理学 2023-11-23 Andrei Constantin , Thomas R. Harvey , Sebastian von Hausegger , Andre Lukas

We consider dynamics of a flat anisotropic Universe filled by a perfect fluid near a cosmological singularity in quadratic gravity. Two possible regimes are described -- the Kasner anisotropic solution and an isotropic "vacuum radiation"…

广义相对论与量子宇宙学 · 物理学 2017-01-04 A. Toporensky , D. Müller

In this manuscript, we investigate the patterns satisfied by the cosmological anisotropy under the hypothesis of the observers being co-moving with a perfect fluid whose induced space sections are homogeneous with vanishing scalar…

广义相对论与量子宇宙学 · 物理学 2021-03-31 Leandro G. Gomes

In this paper we investigate, from the dynamical systems perspective, the evolution of a Kantowski-Sachs metric in a generic class of $f(R)$ models. We present conditions (i. e., differentiability conditions, existence of minima, monotony…

宇宙学与河外天体物理 · 物理学 2014-05-27 Genly Leon , Armando A. Roque

The Standard Cosmological Model assumes that the Universe is, on average, homogeneous and isotropic for large scales (z>1), but this principle has been questioned from the results about Cosmic Microwave Background. This radiation has…

综合物理 · 物理学 2016-04-19 Ericsson López , Mario Llerena , Franklin Aldás

We study the GMGHS spacetimes to analyze the evolution of the anisotropy universe, which can be treated as a doubly warped products manifold possessing warping functions (or scale factor) having the Kantowski-Sachs solution which represents…

广义相对论与量子宇宙学 · 物理学 2016-01-12 Jaedong Choi

Within the context of a cosmic space whose energy source is modeled with a perfect fluid, a uniform model of Universe based on a standard FRW cosmology containing decoupled mixed matter sources namely stiff matter and cosmic dust together…

广义相对论与量子宇宙学 · 物理学 2016-09-07 Denisa-Andreea Mihu

In the context of the modified teleparallel $f(T, B)$-theory of gravity, we consider a homogeneous and anisotropic background geometry described by the Kantowski-Sachs line element. We derive the field equations and investigate the…

广义相对论与量子宇宙学 · 物理学 2022-07-19 Genly Leon , Andronikos Paliathanasis

Cosmological solutions are obtained in an anisotropic Kantowski-Sachs (KS) and Bianchi Type-I universes considering a cosmological constant with Skyrme fluid. Interestingly, the solutions obtained here in both the KS and Bianchi-I…

广义相对论与量子宇宙学 · 物理学 2022-06-09 Rikpratik Sengupta , B C Paul , Prasenjit Pal

We present an exact solution of Einstein equations that describes a Bianchi type III spacetime with conformal expansion. The matter content is given by an anisotropic scalar field and two perfect fluids representing dust and isotropic…

广义相对论与量子宇宙学 · 物理学 2013-11-11 Saulo Carneiro , Guillermo A. Mena Marugan

We consider brane Kantowski-Sachs Universe when bulk space is five-dimensional Anti-deSitter space. The corresponding cosmological equations with perfect fluid are written. For several specific choices of relation between energy and…

广义相对论与量子宇宙学 · 物理学 2007-05-23 A. N. Makarenko , V. V. Obukhov , K. E. Osetrin
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