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The observed accelerating universe indicates the presence of Dark Energy which is probably interpreted in terms of an extremely light gravitational scalar field. We suggest a way to probe this scalar field which contributes to optical…

广义相对论与量子宇宙学 · 物理学 2011-11-03 Yasunori Fujii , Kensuke Homma

Diverse cosmological and astrophysical observations strongly hint at the presence of dark matter and dark energy in the Universe. One of the main goals of Cosmology is to explain the nature of these two components. It may well be that both…

高能物理 - 理论 · 物理学 2023-07-10 Carsten van de Bruck , Gaspard Poulot , Elsa M. Teixeira

We investigate scalar-tensor theories, motivated by dark energy models, in the strong gravity regime around the black hole at the centre of our galaxy. In such theories general relativity is modified since the scalar field couples to…

宇宙学与河外天体物理 · 物理学 2022-01-24 David Benisty , Anne-Christine Davis

This article examines the analytic solutions of isotropic spacetime with the minimal coupling of scalar field and matter in the context of energy-momentum squared gravity. The scalar field includes quintessence and phantom dark energy…

广义相对论与量子宇宙学 · 物理学 2023-06-21 M. Sharif , M. Zeeshan Gul

The work deals with homogeneous and isotropic, flat FRW model of the universe which is filled up with non-interacting dark matter and dark energy to compatible with recent observational evidences. By choosing the dark energy in the form of…

广义相对论与量子宇宙学 · 物理学 2013-05-09 Nilanjana Mahata , Subenoy Chakraborty

Scalar cosmological perturbations are investigated in the framework of a model with interacting dark energy and dark matter. In addition to these constituents, the inhomogeneous Universe is supposed to be filled with the standard…

广义相对论与量子宇宙学 · 物理学 2015-07-24 Maxim Eingorn , Claus Kiefer

We present three distinct types of models of dark energy in the form of a scalar field which is explicitly coupled to dark matter. Our construction draws from the pull-back formalism for fluids and generalises the fluid action to involve…

宇宙学与河外天体物理 · 物理学 2013-10-11 A. Pourtsidou , C. Skordis , E. J. Copeland

The last few decades have provided abundant evidence for physics beyond the two standard models of particle physics and cosmology. As is now known, the by far largest part of our universe's matter/energy content lies in the `dark' and…

广义相对论与量子宇宙学 · 物理学 2024-07-16 Hauke Fischer , Christian Käding , Mario Pitschmann

Cosmology with a three-form field interacting with cold dark matter is considered. In particular, the mass of the dark matter particles is assumed to depend upon the amplitude of the three-form field invariant. In comparison to coupled…

宇宙学与河外天体物理 · 物理学 2015-06-12 Tomi S. Koivisto , Nelson J. Nunes

We study the spherical collapse model in dark energy cosmologies, in which dark energy is modelled as a minimally coupled scalar field. We first follow the standard assumption that dark energy does not cluster on the scales of interest.…

天体物理学 · 物理学 2009-11-10 D. F. Mota , C. van de Bruck

We propose a new model of scalar field dark matter interacting with dark energy. Adopting a fluid description of the dark matter field in the regime of rapid oscillations, we find that the equation of state for dark matter is non-zero and…

宇宙学与河外天体物理 · 物理学 2024-04-17 Gaspard Poulot , Elsa M. Teixeira , Carsten van de Bruck , Nelson J. Nunes

Dark energy equation of state can be effectively described by that of a barotropic fluid. The barotropic fluid model describes the background evolution and the functional form of the equation of state parameter is well constrained by the…

宇宙学与河外天体物理 · 物理学 2018-01-31 Archana Sangwan , Ankan Mukherjee , H. K. Jassal

We study a model of scalar field with a general non-minimal kinetic coupling to itself and to the curvature, and additional coupling to the Gauss Bonnet 4-dimensional invariant. The model presents rich cosmological dynamics and some of its…

高能物理 - 理论 · 物理学 2012-02-01 L. N. Granda

This work is a review of the last results of research on the Scalar Field Dark Matter model of the Universe at cosmological and at galactic level. We present the complete solution to the scalar field cosmological scenario in which the dark…

天体物理学 · 物理学 2015-06-24 T. Matos , F. S. Guzman , L. A. Urena-Lopez , D. Nunez

The work investigate a static, isotropic and almost homogeneous Universe containing a real scalar field modeling the Dark-Energy (quintaessence) interacting with pressureless matter. It is argued that the interaction between matter and the…

广义相对论与量子宇宙学 · 物理学 2007-09-04 Alejandro Cabo Bizet , Alejandro Cabo Montes de Oca

An exact, axially symmetric solution to the Einstein-Klein-Gordon field equations is employed to model the dark matter in spiral galaxies. The extended rotation curves from a previous analysis are used to fit the model and a very good…

天体物理学 · 物理学 2007-05-23 F. S. Guzman , T. Matos , H. Villegas-Brena

In the search for an explanation for the current acceleration of the Universe, scalar fields are the most simple and useful tools to build models of dark energy. This field, however, must in principle couple with the rest of the world and…

广义相对论与量子宇宙学 · 物理学 2016-11-18 Carsten van de Bruck , Jurgen Mifsud , José P. Mimoso , Nelson J. Nunes

The problem of dark energy can be roughly stated as the proposition and validation of a cosmological model that can explain the phenomenon of the accelerated expansion of the Universe. This problem is an open discussion topic in modern…

广义相对论与量子宇宙学 · 物理学 2014-12-19 Genly Leon

We consider a scalar-tensor theory of gravitation with the scalar source being the trace of the stress-energy tensor of the scalar field itself and matter. We obtain an example of a numerical solution of the cosmological equations which…

广义相对论与量子宇宙学 · 物理学 2016-10-05 I. G. Dudko , Yu. P. Vyblyi

In this paper we study the possibility of building models of dark energy with equation of state across -1 and propose explicitly a model with a single scalar field which gives rise to an equation of state larger than -1 in the past and less…

高能物理 - 唯象学 · 物理学 2009-11-11 Mingzhe Li , Bo Feng , Xinmin Zhang
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