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相关论文: A Model for Cosmic Self-Acceleration

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An explicitly covariant formulation is presented of a modified DGP scenario proposed recently [1], to avoid the instability of the self-accelerating branch. It is based on the introduction of a bulk scalar field with appropriate non-minimal…

高能物理 - 理论 · 物理学 2008-11-26 Alexey S. Koshelev , Theodore N. Tomaras

We consider the model of modified gravity with dynamical torsion. This model was found to have promising stability properties about various backgrounds. The model admits a self-accelerating solution. We have shown previously that if the…

高能物理 - 理论 · 物理学 2018-03-28 V. Nikiforova

I review a class of nonlocally modified gravity models which were proposed to explain the current phase of cosmic acceleration without dark energy. Among the topics considered are deriving causal and conserved field equations, adjusting the…

宇宙学与河外天体物理 · 物理学 2015-06-18 R. P. Woodard

It is shown here that a dynamical Planck mass can drive the scale factor of the universe to accelerate. The negative pressure which drives the cosmic acceleration is identified with the unusual kinetic energy density of the Planck field. No…

广义相对论与量子宇宙学 · 物理学 2010-11-01 Janna Levin

There is now overwhelming observational evidence that our Universe is accelerating in its expansion. I discuss how modified gravitational models can provide an explanation for this observed late-time cosmic acceleration. We consider…

天体物理学 · 物理学 2008-11-26 Damien A. Easson

We consider a model belonging to the class of gravities with dynamical torsion. The model is free of ghosts and gradient instabilities about Minkowski and torsionless Einstein backgrounds. We find that at zero cosmological constant, the…

高能物理 - 理论 · 物理学 2017-10-19 V. Nikiforova , S. Randjbar-Daemi , V. Rubakov

We present a cosmological model with a solution that self-accelerates at late-times without signs of ghost instabilities on small scales. The model is a natural extension of the Brans-Dicke (BD) theory including a non-linear derivative…

宇宙学与河外天体物理 · 物理学 2010-01-08 Fabio P Silva , Kazuya Koyama

A novel, interesting class of scalar-tensor gravity theories is those with a limit on the field motion, where the scalar field either goes to a constant acceleration or stops accelerating and goes to a constant velocity. We combine these…

广义相对论与量子宇宙学 · 物理学 2022-11-02 Eric V. Linder

The notion of self-acceleration has been introduced as a convenient way to theoretically distinguish cosmological models in which acceleration is due to modified gravity from those in which it is due to the properties of matter or fields.…

宇宙学与河外天体物理 · 物理学 2020-01-22 Luca Amendola , Valeria Pettorino

New corrections to General Relativity are considered in the context of modified $f(R)$ gravity, that satisfy cosmological and local gravity constraints. The proposed models behave asymptotically as $R-2\Lambda$ at large curvature and show…

广义相对论与量子宇宙学 · 物理学 2022-01-13 L. N. Granda

We show how to construct consistent braneworld models which exhibit late time acceleration. Unlike self-acceleration, which has a de Sitter vacuum state, our models have the standard Minkowski vacuum and accelerate only in the presence of…

高能物理 - 理论 · 物理学 2009-04-17 Christos Charmousis , Ruth Gregory , Antonio Padilla

Within the framework of the recently proposed ghost-free massive gravity, a cosmological constant-type self-accelerating solution has been obtained for Minkowski and de Sitter reference metrics. We ease the assumption on the reference…

高能物理 - 理论 · 物理学 2012-10-15 Hayato Motohashi , Teruaki Suyama

The DGP brane-world model provides a simple alternative to the standard LCDM cosmology, with the same number of parameters. There is no dark energy - the late universe self-accelerates due to an infrared modification of gravity. We compute…

天体物理学 · 物理学 2008-11-26 Roy Maartens , Elisabetta Majerotto

I examine how two specific examples of modified gravity explanations of cosmic acceleration help us understand some general problems confronting cosmological tests of gravity: how do we distinguish modified gravity from dark energy if they…

宇宙学与河外天体物理 · 物理学 2009-11-05 Wayne Hu

The observed acceleration of the Universe can be explained by modifying general relativity. One such attempt is the nonlocal model of Deser and Woodard. Here we fix the background cosmology using results from the Planck satellite and…

宇宙学与河外天体物理 · 物理学 2014-09-05 Scott Dodelson , Sohyun Park

We propose a cosmological model which exhibits the phenomenon of self-acceleration: the Universe is attracted to the phase of accelerated expansion at late times even in the absence of the cosmological constant. The self-acceleration is…

高能物理 - 理论 · 物理学 2008-04-15 D. S. Gorbunov , S. M. Sibiryakov

The current standard cosmological model is constructed within the framework of general relativity with a cosmological constant $\Lambda$, which is often associated with dark energy, and phenomenologically explains the accelerated cosmic…

广义相对论与量子宇宙学 · 物理学 2023-06-27 Jiamin Hou , Julian Bautista , Maria Berti , Carolina Cuesta-Lazaro , César Hernández-Aguayo , Tilman Tröster , Jinglan Zheng

With the advent of gravitational-wave astronomy marked by the aLIGO GW150914 and GW151226 observations, a measurement of the cosmological speed of gravity will likely soon be realized. We show that a confirmation of equality to the speed of…

宇宙学与河外天体物理 · 物理学 2017-01-02 Lucas Lombriser , Nelson A. Lima

The recent observational data in cosmology seem to indicate that the universe is currently expanding in an accelerated way. An intriguing interpretation of these data is that they may just be signalling that Einstein's General Relativity is…

高能物理 - 理论 · 物理学 2018-05-18 Fulvio Sbisà

In 'modified' gravity the observed acceleration of the universe is explained by changing the gravitational force law or the number of degrees of freedom in the gravitational sector. Both possibilities can be tested by measurements of…

宇宙学与河外天体物理 · 物理学 2017-12-27 Clare Burrage , David Parkinson , David Seery
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