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The dynamical consequences of a bimetric scalar-tensor theory of gravity with a dynamical light speed are investigated in a cosmological setting. The model consists of a minimally-coupled self-gravitating scalar field coupled to ordinary…

广义相对论与量子宇宙学 · 物理学 2009-11-07 M. A. Clayton , J. W. Moffat

Massive gravity with second and fourth derivatives is shown to give both attractive and repulsive gravities. In contrast to the attractive gravity correlated with the energy-momentum tensor, the repulsive gravity is related to a fixed mass…

天体物理学 · 物理学 2007-05-23 Xiang-Song Chen

We constrain the contribution of tensor-mode perturbations with free $n_t$ in the models with dynamical dark energy with the barotropic equation of state using Planck-2015 data on CMB anisotropy, polarization and lensing, BICEP2/Keck Array…

宇宙学与河外天体物理 · 物理学 2017-06-15 O. Sergijenko

Recent observations provide strong evidence that the universe is accelerating. This confronts theory with a severe challenge. Explanations of the acceleration within the framework of general relativity are plagued by difficulties. General…

天体物理学 · 物理学 2008-11-26 Roy Maartens

We present a class of exact scalar-tensor black holes for a shift-symmetric part of the Horndeski action. The action includes a higher order scalar tensor interaction term. We find that for a static and spherically symmetric space-time, the…

广义相对论与量子宇宙学 · 物理学 2014-09-11 Eugeny Babichev , Christos Charmousis

We have investigated a brane world model in which the gravitational field in the bulk is described both by a metric tensor and a minimally coupled scalar field. This scalar field is taken to be a chameleon with an appropriate potential…

广义相对论与量子宇宙学 · 物理学 2017-12-12 Y. Bisabr , F. Ahmadi

Theories with a pole in the kinetic term have been used to great effect in studying inflation, owing to their quantum stability and attractor properties. We explore the use of such pole kinetic terms in dark energy theories, finding an…

宇宙学与河外天体物理 · 物理学 2020-01-15 Eric V. Linder

The theories of brane world and multidimensional gravity are widely discussed in the literature in connection with problems of evolution of early Universe, including dark matter and energy. A natural physical concept is that a distinguished…

广义相对论与量子宇宙学 · 物理学 2009-10-12 Boris E. Meierovich

The energy density of the universe today may be dominated by the vacuum energy of a slowly rolling scalar field. Making a quantum expansion around such a time dependent solution is found to break fundamental symmetries of quantum field…

高能物理 - 唯象学 · 物理学 2008-11-26 Pankaj Jain , Subhadip Mitra

We analyze solutions to Friedmann-Robertson-Walker cosmologies in Brans-Dicke theory, where a scalar field is coupled to gravity. Matter is modelled by a $\gamma$-law perfect fluid, including false-vacuum energy as a special case. Through a…

广义相对论与量子宇宙学 · 物理学 2011-07-19 Shawn J. Kolitch , Douglas M. Eardley

We investigate emergent gravity extending the paradigm of the AdS/CFT correspondence. The emergent graviton is associated to the (dynamical) expectation value of the energy-momentum tensor. We derive the general effective description of…

高能物理 - 理论 · 物理学 2023-02-28 Panos Betzios , Elias Kiritsis , Vasilis Niarchos

In this work, we demonstrate that a dynamical dark energy component predicted by massive gravity gives rise to a distinctive evolution of the equation of state. This scenario is favoured over the standard $\Lambda$CDM model when confronted…

宇宙学与河外天体物理 · 物理学 2025-05-27 Juri Smirnov

Scalar fields coupled to gravity via $\xi R {\Phi}^2$ in arbitrary Friedmann-Robertson-Walker backgrounds can be represented by an effective flat space field theory. We derive an expression for the scalar energy density where the effective…

广义相对论与量子宇宙学 · 物理学 2009-10-28 David Hochberg , Thomas W. Kephart

We consider scalar perturbations of energy--density for a class of cosmological models where an early phase of accelerated expansion evolves, without any fine--tuning for graceful exit, towards the standard Friedman eras of observed…

广义相对论与量子宇宙学 · 物理学 2007-05-23 S. Capozziello , G. Lambiase , G. Scarpetta

We study the interaction between dark matter and dark energy, with dark energy described by a scalar field having a double exponential effective potential. We discover conditions under which such a scalar field driven solution is a late…

广义相对论与量子宇宙学 · 物理学 2015-08-06 Vartika Gupta , Rakesh Kabir , Amitabha Mukherjee , Daksh Lohiya

The properties of dynamical Dark Energy (DE) and, in particular, the possibility that it can form or contribute to stable inhomogeneities, have been widely debated in recent literature, also in association to a possible coupling between DE…

天体物理学 · 物理学 2014-11-18 Roberto Mainini

The dynamical properties of a model of dark energy in which two scalar fields are coupled by a non-canonical kinetic term are studied. We show that overall the addition of the coupling has only minor effects on the dynamics of the two-field…

宇宙学与河外天体物理 · 物理学 2014-11-20 Carsten van de Bruck , Joel M. Weller

A new phenomenological dark energy model, originally associated to the large-scale structure formation and considered as a solution to the fine-tuning and coincidence problems related to the cosmological constant, was analyzed within the…

广义相对论与量子宇宙学 · 物理学 2026-03-05 A. Kazım Çamlıbel

We explore general scalar-tensor models in the presence of a kinetic mixing between matter and the scalar field, which we call Kinetic Matter Mixing. In the frame where gravity is de-mixed from the scalar this is due to disformal couplings…

宇宙学与河外天体物理 · 物理学 2017-02-15 Guido D'Amico , Zhiqi Huang , Michele Mancarella , Filippo Vernizzi

When coupling fermions to gravity, torsion is naturally induced. We consider the possibility that fermion bilinears can act as a source for torsion, altering the dynamics of the early universe such that the big bang gets replaced with a…

广义相对论与量子宇宙学 · 物理学 2017-11-08 Shane Farnsworth , Jean-Luc Lehners , Taotao Qiu
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