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We study a model of a scalar field minimally coupled to gravity, with a specific potential energy for the scalar field, and include curvature and radiation as two additional parameters. Our goal is to obtain analytically the complete set of…

高能物理 - 理论 · 物理学 2013-05-30 Itzhak Bars , Shih-Hung Chen , Paul J. Steinhardt , Neil Turok

The problem of classification of exact solutions of Maxwell's vacuum equations for admissible electromagnetic fields and homogeneous space-time with the group of motions $G_3(VIII)$ according to the Bianchi classification is considered. All…

广义相对论与量子宇宙学 · 物理学 2023-03-06 V. V. Obukhov

We study Bianchi cosmologies in the ghost-free bigravity theory assuming both metrics to be homogeneous and anisotropic, of the Bianchi class A, which includes types I,II,VI$_0$,VII$_0$,VIII, and IX. We assume the universe to contain a…

高能物理 - 理论 · 物理学 2013-11-08 Kei-ichi Maeda , Mikhail S. Volkov

Why is the Universe so homogeneous and isotropic? We summarize a general study of a $\gamma$-law perfect fluid alongside an inhomogeneous, massless scalar gauge field (with homogeneous gradient) in anisotropic spaces with General…

广义相对论与量子宇宙学 · 物理学 2019-09-27 Ben David Normann , Sigbjørn Hervik , Angelo Ricciardone , Mikjel Thorsrud

We consider the asymptotic dynamics of the Einstein-Maxwell field equations for the class of non-tilted Bianchi cosmologies with a barotropic perfect fluid and a pure homogeneous source-free magnetic field, with emphasis on models of…

广义相对论与量子宇宙学 · 物理学 2009-11-10 J. T. Horwood , J. Wainwright

Self-consistent solutions to nonlinear spinor field equations in General Relativity have been studied for the case of Bianchi type-I space-time filled with perfect fluid. The initial and the asymptotic behavior of the field functions and…

广义相对论与量子宇宙学 · 物理学 2009-10-28 B. Saha , G. N. Shikin

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

In order to find out whether empty singular boundaries can arise in higher dimensional Gravity, we study the solution of Einstein's equations consisting in a ($N+2$)-dimensional static and hyperplane symmetric perfect fluid satisfying the…

广义相对论与量子宇宙学 · 物理学 2012-08-21 Ricardo E. Gamboa Saravi

In this work the possible geodesic completeness of an electromagnetic dipole wormhole is studied in detail. The space-time contains a curvature singularity and belongs to a class of solutions to the Einstein-Maxwell equations with a coupled…

广义相对论与量子宇宙学 · 物理学 2023-03-23 Juan Carlos Del Águila , Tonatiuh Matos

We study the isotropisation of the homogeneous but anisotropic Bianchi class A models in presence of a minimally coupled and massive scalar field with or without a perfect fluid. To this end, we use the Hamiltonian formalism of Arnowitt,…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Stephane Fay

The global properties of spatially homogeneous cosmological models with collisionless matter are studied. It is shown that as long as the mean curvature of the hypersurfaces of homogeneity remains finite no singularity can occur in finite…

广义相对论与量子宇宙学 · 物理学 2009-10-22 Alan D. Rendall

Singularity theorems demonstrate the inevitable breakdown of the concept of continuous, classical spacetime under highly general conditions. Quantum gravity is expected to intervene to avoid singularities and models so far hint towards…

广义相对论与量子宇宙学 · 物理学 2024-08-30 Raúl Carballo-Rubio , Stefano Liberati , Vania Vellucci

Some new exact solutions of Einstein's field equations have come forth within the scope of a spatially homogeneous and anisotropic Bianchi type-III space-time filled with barotropic fluid and dark energy by considering a variable…

宇宙学与河外天体物理 · 物理学 2014-03-20 Hassan Amirhashchi , Anirudh Pradhan , Rekha Jaiswal

We explore the phase-space of homogeneous and anisotropic spacetimes within symmetric teleparallel $f(Q)$-gravity. Specifically, we consider the Kantowski-Sachs and locally rotational Bianchi III geometries to describe the physical space.…

广义相对论与量子宇宙学 · 物理学 2024-03-12 Alfredo D. Millano , K. Dialektopoulos , N. Dimakis , A. Giacomini , H. Shababi , Amlan Halder , A. Paliathanasis

In one-loop string effective action, we study a generality of non-singular cosmological solutions found in the isotropic and homogeneous case. We discuss Bianchi I and IX type spacetimes. We find that nonsingular solutions still exist in…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Hiroki Yajima , Kei-ichi Maeda , Hidetoshi Ohkubo

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

Homogeneous, nearly-isotropic Bianchi cosmological models are considered. Their time evolution is expressed as a complete set of non-interacting linear modes on top of a Friedmann-Robertson-Walker background model. This connects the…

广义相对论与量子宇宙学 · 物理学 2011-09-08 Andrew Pontzen , Anthony Challinor

We present a class of graviton-dilaton models in which a homogeneous isotropic universe, such as our observed one, evolves with no singularity at any time. Such models may stand on their own as interesting models for singularity free…

高能物理 - 理论 · 物理学 2009-10-30 S. Kalyana Rama

Generic resolution of singularities and geodesic completeness in the loop quantization of Bianchi-II spacetimes with arbitrary minimally coupled matter is investigated. Using the effective Hamiltonian approach, we examine two available…

广义相对论与量子宇宙学 · 物理学 2017-12-06 Sahil Saini , Parampreet Singh

Exact electromagnetic wave solutions to Maxwell equations on anisotropic Bianchi I cosmological spacetime backgrounds are studied. The waves evolving on Bianchi I spacetimes exhibit birefringence (associated to linear polarization) and…

广义相对论与量子宇宙学 · 物理学 2017-08-23 Felipe A. Asenjo , Sergio A. Hojman
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