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相关论文: Cosmic acceleration, scalar fields and observation…

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We consider cosmological constraints arising from the background expansion history on the ef- fective field theory of cosmic acceleration, a theoretical framework that allows for a unified way to classify both models of dark energy and…

宇宙学与河外天体物理 · 物理学 2013-04-10 Eva-Maria Mueller , Rachel Bean , Scott Watson

If our Universe is allowed to absorb baby universes, one obtains a modified Friedmann equation that can explain the late time acceleration of our Universe and there is no need for a cosmological constant. In addition the modified Friedmann…

广义相对论与量子宇宙学 · 物理学 2024-01-17 Jan Ambjorn , Yoshiyuki Watabiki

We show that the scalar-vacuum Brans-Dicke equations in 5D are equivalent to Brans-Dicke theory in 4D with a self interacting potential and an effective matter field. The cosmological implication, in the context of FRW models, is that the…

广义相对论与量子宇宙学 · 物理学 2010-04-30 J. Ponce de Leon

We use action-angle variables to describe the basic physics of coherent scalar field oscillations in the expanding universe. These analytical mechanics methods have some advantages, like the identification of adiabatic invariants. As an…

天体物理学 · 物理学 2016-08-30 Eduard Masso , Francesc Rota , Gabriel Zsembinszki

In this work, I develop an alternative explanation for the acceleration of the cosmic expansion, which seems to be a result of recent high redshift Supernova data. In the current interpretation, this cosmic acceleration is explained by…

广义相对论与量子宇宙学 · 物理学 2007-05-23 J. -F. Pascual-Sánchez

The solution to the current extending Universe problem, and the description of all stages of evolution compels scientists to consider various cosmological models. Scalar - tensor models are rather simple and also allow us to clearly define…

广义相对论与量子宇宙学 · 物理学 2015-06-23 K. E. Osetrin , A. N. Makarenko , Yu. A. Rybalov

We often find in the literature solutions to the Friedmann and fluid equations for simple cosmological models during the matter, radiation or cosmological constant dominated epochs. However no solutions appear for the inflationary era…

广义相对论与量子宇宙学 · 物理学 2020-07-30 Gabriel German

We consider the emergence of large-scale cosmological expansion in scalar-tensor theories of gravity. This is achieved by modelling sub-horizon regions of space-time as weak-field expansions around Minkowski space, and then subsequently…

广义相对论与量子宇宙学 · 物理学 2025-10-15 Chad Briddon , Timothy Clifton , Pierre Fleury

This is a pedagogical review of the recent observational data obtained from type Ia supernova surveys that support the accelerating expansion of the universe. The methods for the analysis of the data are reviewed and some of the theoretical…

天体物理学 · 物理学 2007-05-23 L. Perivolaropoulos

The observed late-time acceleration of the cosmic expansion constitutes a fundamental problem in modern theoretical physics and cosmology. In an attempt to weight the validity of a large number of dark energy models, I use the recent…

宇宙学与河外天体物理 · 物理学 2010-01-21 Spyros Basilakos

A central theme in cosmology is the perplexing fact that the Universe is undergoing an accelerating expansion. The latter, one of the most important and challenging current problems in cosmology, represents a new imbalance in the governing…

广义相对论与量子宇宙学 · 物理学 2011-09-28 Francisco S. N. Lobo

An accelerating flat universe with a variable cosmological term is obtained in the Robertson-Walker metric. The variable cosmological term is defined by the correction terms of the metric tensor field. Simple solutions of the scale factor…

天体物理学 · 物理学 2015-06-24 Takao Fukui

Emergent scenario of cosmic evolution is a topic of great interest in recent cosmology, especially because it describes a non-singular origin of the Universe unlike the Big-Bang models. This types of cosmic evolution pattern have already…

广义相对论与量子宇宙学 · 物理学 2023-09-01 Subhayan Maity , Sujayita Bakra

In this paper we consider a model of scalar-tensor theory of gravitation in which the scalar field, $\phi$ determines the gravitational coupling G and has a Lagrangian of the form, $\mathcal{L}_{\phi} =-V(\phi)\sqrt{1 -…

广义相对论与量子宇宙学 · 物理学 2008-12-11 Sanil Unnikrishnan , T. R. Seshadri

We describe an accelerating universe model in the context of a scalar-tensor theory. This model is intrinsically closed, and is filled with quintessence-like scalar field components, in addition to the Cold Dark Matter component. With a…

天体物理学 · 物理学 2009-11-10 Sergio del Campo , Patricio Salgado

We explore a cosmological model in which the time scale is variable with the expansion of the universe and the effective spacetime is driven by the inflaton field. An example is considered and their predictions are contrasted between Planck…

广义相对论与量子宇宙学 · 物理学 2019-01-30 Juan Ignacio Musmarra , Mariano Anabitarte , Mauricio Bellini

In this work the accelerated-decelerated transition in a primordial Universe is investigated by using the dynamics of fermion fields within the context of Einstein-Cartan theory, where apart from the curvature the space-time is also…

广义相对论与量子宇宙学 · 物理学 2010-11-19 Marlos O. Ribas , Gilberto M. Kremer

It is well known that interstellar travel is bounded by the finite speed of light, but on very large scales any rocketeer would also need to consider the influence of cosmological expansion on their journey. This paper examines accelerated…

宇宙学与河外天体物理 · 物理学 2015-05-14 Juliana Kwan , Geraint F. Lewis , J. Berian James

We show by using the method of matched asymptotic expansions that a sufficient condition can be derived which determines when a local experiment will detect the cosmological variation of a scalar field which is driving the spacetime…

广义相对论与量子宇宙学 · 物理学 2008-11-26 John D. Barrow , Douglas J. Shaw

A brief account of the current cosmological observations is given and their implications for QCDM and $\Lambda$CDM cosmologies are discussed. The nucleosynthesis and the galaxy formation constraints have been used to put limits on…

天体物理学 · 物理学 2007-05-23 Vinod B. Johri