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相关论文: Accelerating Hilbert-Einstein universe without dyn…

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We propose an explanation for the present accelerated expansion of the universe that does not invoke dark energy or a modification of gravity and is firmly rooted in inflationary cosmology.

高能物理 - 理论 · 物理学 2007-05-23 Edward W. Kolb , Sabino Matarrese , Alessio Notari , Antonio Riotto

A new model of accelerating expansion of the universe is presented. A de Sitter solution in vacuum and a exact solution with the dust mater source are obtained. A new explanation of the acceleration of the cosmic expansion is given. In is…

综合物理 · 物理学 2013-01-16 G. Y. Chee

The kinematics and dynamic interpretation of the cosmological expansion is reviewed in a widely accessible manner with emphasis on the acceleration aspect. Virtually all the approaches that can in principle account for the accelerated…

宇宙学与河外天体物理 · 物理学 2012-10-19 Yu. L. Bolotin , O. A. Lemets , D. A. Yerokhin

Observations show that the expansion of the Universe is accelerating. This requires that the dominant constituent of matter in the Universe has some unusual properties like negative pressure. This exotic component has been given the name…

科普物理 · 物理学 2019-01-17 Manvendra Pratap Rajvanshi , Tuneer Chakraborty , J. S. Bagla

It is the common consensus that the expansion of a universe always slows down if the gravity provided by the energy sources therein is attractive and accordingly one needs to invoke dark energy as a source of anti-gravity for understanding…

天体物理学 · 物理学 2008-11-26 Chia-Hsun Chuang , Je-An Gu , W-Y. P. Hwang

In this work we consider the possibility of describing the current evolution of the universe, without the introduction of any cosmological constant or dark energy (DE), by modifying the Einstein-Hilbert (EH) action. In the context of the…

广义相对论与量子宇宙学 · 物理学 2009-11-11 A. de la Cruz-Dombriz , A. Dobado

No. It is simply not plausible that cosmic acceleration could arise within the context of general relativity from a back-reaction effect of inhomogeneities in our universe, without the presence of a cosmological constant or ``dark energy.''…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Akihiro Ishibashi , Robert M. Wald

The discovery ten years ago that the expansion of the Universe is accelerating put in place the last major building block of the present cosmological model, in which the Universe is composed of 4% baryons, 20% dark matter, and 76% dark…

天体物理学 · 物理学 2009-02-27 Joshua Frieman , Michael Turner , Dragan Huterer

We perform large-scale cosmological simulations that solve Einstein's equations directly via numerical relativity. Starting with initial conditions sampled from the cosmic microwave background, we track the emergence of a cosmic web without…

宇宙学与河外天体物理 · 物理学 2019-03-27 Hayley J. Macpherson , Daniel J. Price , Paul D. Lasky

The discovery ten years ago that the expansion of the Universe is accelerating put in place the present cosmological model, in which the Universe is composed of 4% baryons, 20% dark matter, and 76% dark energy. Yet the underlying cause of…

宇宙学与河外天体物理 · 物理学 2009-04-17 Joshua A. Frieman

The present day accelerated expansion of the universe is naturally addressed within the Brans-Dicke theory just by using holographic dark energy model with inverse of Hubble scale as IR cutoff. It is also concluded that if the universe…

广义相对论与量子宇宙学 · 物理学 2015-05-13 Bibekananda Nayak , Lambodar Prasad Singh

I show that a generic quantum phenomenon can drive cosmic acceleration without the need for dark energy or modified gravity. When treating the universe as a quantum system, one typically focuses on the scale factor (of an FRW spacetime) and…

广义相对论与量子宇宙学 · 物理学 2019-09-13 Luke M. Butcher

We show that the current accelerated expansion of the Universe can be explained without resorting to dark energy. Models of generalized modified gravity, with inverse powers of the curvature can have late time accelerating attractors…

天体物理学 · 物理学 2008-11-26 Olga Mena , Jose Santiago , Jochen Weller

An attempt is made to explain the spiral structure of spiral galaxies through a possible rotation of the Universe. To this end, we write down a possible form of the metric, and we calculate the necessary quantities (Rik, Tik, ...) in order…

天体物理学 · 物理学 2009-04-27 Evangelos Chaliasos

Acceleration of the universe is obtained from a model of non-relativistic particles with a short-range attractive interaction, at low enough temperature to produce a Bose-Einstein condensate. Conditions are derived for negative-pressure…

天体物理学 · 物理学 2015-05-13 German Izquierdo , Jaime Besprosvany

Einstein-Cartan theory is an extension of the standard formulation of General Relativity characterized by a non-vanishing torsion. The latter is sourced by the matter fields via the spin tensor, and its effects are expected to be important…

广义相对论与量子宇宙学 · 物理学 2020-10-08 Francisco Cabral , Francisco S. N. Lobo , Diego Rubiera-Garcia

The free parameters of a flat accelerating model without dark energy are constrained by using Supernovae type Ia and observational H(z) data. Instead of the vacuum dominance, the present accelerating stage in this modified Einstein-de…

宇宙学与河外天体物理 · 物理学 2016-11-15 R. C. Santos , F. E. Silva , J. A. S. Lima

To describe dark energy we introduce a fluid model with no free parameter on the microscopic level. The constituents of this fluid are massless particles which are a dynamical realisation of the unextended $D=(3+1)$ Galilei algebra. These…

宇宙学与河外天体物理 · 物理学 2009-10-29 P. C. Stichel , W. J. Zakrzewski

We suggest an interpretation of Einstein Equations of General Relativity at large scales in which the Cosmological constant is exactly zero in the limit of zero spacetime variations of fundamental constants. We argue that in a…

高能物理 - 理论 · 物理学 2018-02-09 Denis Bashkirov

It is postulated in Einstein's relativity that the speed of light in vacuum is a constant for all observers. However, the effect of quantum gravity could bring an energy dependence of light speed. Even a tiny speed variation, when amplified…

高能物理 - 唯象学 · 物理学 2016-07-28 Haowei Xu , Bo-Qiang Ma