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Maxwell electrodynamics, considered as a source of the classical Einstein field equations, leads to the singular isotropic Friedmann solutions. We show that this singular behavior does not occur for a class of nonlinear generalizations of…

广义相对论与量子宇宙学 · 物理学 2007-05-23 V. A. De Lorenci , R. Klippert , M. Novello , J. M. Salim

We apply the dynamical systems tools to study the (linear) dynamics of Friedmann-Robertson-Walker universes that are fuelled by non-linear electrodynamics. We focus, mainly, in two particular models. In the first model the cosmic evolution…

广义相对论与量子宇宙学 · 物理学 2009-05-08 Ricardo Garcia-Salcedo , Tame Gonzalez , Claudia Moreno , Israel Quiros

The possibility to avoid the cosmic initial singularity as a consequence of nonlinear effects on the Maxwell eletromagnetic theory is discussed. For a flat FRW geometry we derive the general nonsingular solution supported by a magnetic…

天体物理学 · 物理学 2009-11-10 C. S. Camara , M. R. de Garcia Maia , J. C. Carvalho , J. A. S. Lima

We study inflation and late-time acceleration in the expansion of the universe in non-minimal electromagnetism, in which the electromagnetic field couples to the scalar curvature function. It is shown that power-law inflation can be…

天体物理学 · 物理学 2009-06-23 Kazuharu Bamba , Sergei D. Odintsov

Nonlinear electrodynamics with two dimensional parameters is studied. The range of electromagnetic fields when principles of causality, unitarity and the classical stability hold, are obtained. A singularity of the electric field at the…

广义相对论与量子宇宙学 · 物理学 2022-12-27 S. I. Kruglov

A new model of nonlinear electrodynamics with a dimensional parameter $\beta$ coupled to gravity is considered. We show that an accelerated expansion of the universe takes place if the nonlinear electromagnetic field is the source of the…

广义相对论与量子宇宙学 · 物理学 2016-01-26 S. I. Kruglov

We study the expansion of the Universe using an effective Friedmann equation obtained from the dynamics of GFT (Group Field Theory) isotropic condensates. The evolution equations are classical, with quantum correction terms to the Friedmann…

广义相对论与量子宇宙学 · 物理学 2016-11-24 Marco de Cesare , Mairi Sakellariadou

In the framework of a flat Friedmann-Lema{\^\i}tre-Robertson-Walker (FLRW) geometry, we present a nonsingular model (no big bang singularity at finite time) of our universe describing its evolution starting from its early inflationary era…

广义相对论与量子宇宙学 · 物理学 2016-04-20 Jaume de Haro , Jaume Amorós , Supriya Pan

A new model of nonlinear electrodynamics with dimensional parameters $\beta$ and $\gamma$ is proposed. The principles of causality and unitarity are studied. We show that a singularity of the electric field at the origin of charges is…

广义相对论与量子宇宙学 · 物理学 2020-04-29 S. I. Kruglov

The energy-momentum tensor coming from one-parameter effective Yang- Mills theory is here used to describe the matter-energy content of the homogeneous and isotropic Friedmann cosmology in its early stages. The behavior of all solutions is…

广义相对论与量子宇宙学 · 物理学 2010-02-25 Vitorio A. De Lorenci

The cosmological solutions of the non-minimal $ Y (R)F^2 $ theory which are compatible with FRW space-time are investigated. In order to avoid the isotropy violation of a vector field, it can be considered that the presence of a triplet of…

广义相对论与量子宇宙学 · 物理学 2019-12-24 Özcan Sert

In this paper, we examine a flat FLRW spacetime with a scalar field potential and show by applying Osgood's criterion to the Einstein field equations that all such models, irrespective of the particular choice of potential develop…

广义相对论与量子宇宙学 · 物理学 2016-04-26 Ikjyot Singh Kohli

A stiff matter-dominated universe modeled by a free massless scalar field minimally coupled to gravity in a Friedmann-Lema\^{\i}tre-Robertson-Walker (FLRW) geometry is quantized. Generalized complex-width gaussian superpositions of the…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Felipe T. Falciano , Nelson Pinto-Neto , E. Sergio Santini

A model of nonlinear electrodynamics with a dimensional parameter $\beta$ is considered. Electromagnetic fields are the source of the gravitation field and inflation of the universe. We imply that the universe is filled by stochastic…

广义相对论与量子宇宙学 · 物理学 2017-05-08 S. I. Kruglov

Simple exact solutions presented here describe the universes which spatial geometries are asymptotically homogeneous and isotropic near the initial singularity, but which evolution goes under the influence of primordial magnetic fields. In…

宇宙学与河外天体物理 · 物理学 2013-12-19 G. A. Alekseev

In this paper, we study the model of the late universe with the homogeneous, isotropic and flat Friedmann-Robertson-Walker metric, where the source of the gravitational field is based on the fermion and boson field, with the Maxwell term…

广义相对论与量子宇宙学 · 物理学 2020-07-13 O. Razina , P. Tsyba , B. Meirbekov , R. Myrzakulov

A general class of cosmological models driven by a nonlocal scalar field inspired by the string field theory is studied. Using the fact that the considering linear nonlocal model is equivalent to an infinite number of local models we have…

高能物理 - 理论 · 物理学 2008-11-26 I. Ya. Aref'eva , L. V. Joukovskaya , S. Yu. Vernov

A new model of nonlinear electromagnetic fields possessing a dimensional parameter $\beta$ is proposed. Electromagnetic fields are considered as the source of the gravitation field and accelerated expansion of the universe is driven by…

广义相对论与量子宇宙学 · 物理学 2016-03-25 S. I. Kruglov

In this paper, we consider a nonminimal coupling model between gravity and nonlinear electrodynamics with cosmological constant. This cosmological model is designed to account for both the inflationary epoch of the early universe and the…

广义相对论与量子宇宙学 · 物理学 2024-10-10 Chilwatun Nasiroh , Ramy F. Izzah , Fiki T. Akbar , Bobby E. Gunara

We study the non-linear dynamics of quantum fields in matter and radiation dominated universes, using the non-equilibrium field theory approach combined with the non-perturbative Hartree and the large N approximations. We examine the…

高能物理 - 唯象学 · 物理学 2014-11-17 D. Boyanovsky , D. Cormier , H. J. de Vega , R. Holman , A. Singh , M. Srednicki
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