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相关论文: Quintessence at Galactic Level?

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In this article we describe a model of the universe consisting of a mixture of the ordinary matter and a so-called cosmic quaternionic field. The basic idea here consists in an attempt to interpret $\Lambda$ as the energy density of the…

天体物理学 · 物理学 2008-11-26 V. Majernik

The two most popular candidates for dark energy, i.e. a cosmological constant and quintessence, are very difficult to distinguish observationally, mostly because the quintessence field does not have sizable fluctuations. We study a scalar…

天体物理学 · 物理学 2009-11-11 Massimo Pietroni

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 investigate if the fluctuations of the scalar field mediating quintessence -- the cosmon -- can play an important role in cosmology. Small fluctuations with short wavelength behave similar to a relativistic gas. In contrast, the…

高能物理 - 唯象学 · 物理学 2009-11-07 C. Wetterich

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

This review considers the theoretical approaches to the understanding of dark energy which comprises approximately 68\% of the energy of our Universe and explains an acceleration in its expansion. Following a discussion of the main approach…

广义相对论与量子宇宙学 · 物理学 2024-03-12 Galina L. Klimchitskaya , Vladimir M. Mostepanenko

Quintessence is a canonical scalar field introduced to explain the late-time cosmic acceleration. The cosmological dynamics of quintessence is reviewed, paying particular attention to the evolution of the dark energy equation of state w.…

广义相对论与量子宇宙学 · 物理学 2015-06-15 Shinji Tsujikawa

Dynamical vacuum energy or quintessence, a slowly varying and spatially inhomogeneous component of the energy density with negative pressure, is currently consistent with the observational data. One potential difficulty with the idea of…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Takeshi Chiba

Brans--Dicke scalar--tensor theory provides a conformally coupling of the scalar field with gravity in Einstein's frame. This model is equivalent to an interacting quintessence in which dark matter is coupled to dark energy. This provides a…

广义相对论与量子宇宙学 · 物理学 2015-05-30 Fatimah Shojai , Ali Shojai

We review the gauged quintessence scenario, wherein the quintessence scalar field responsible for dark energy is promoted to a complex field charged under a dark $U(1)$ gauge symmetry. This construction leads to new and potentially rich…

高能物理 - 唯象学 · 物理学 2025-08-08 Kunio Kaneta , Hye-Sung Lee , Jiheon Lee , Jaeok Yi

We discuss the possibility that dark energy arises from a strongly-coupled Higgs-Yang-Mills set of interacting fields in the non-perturbative regime. We choose the simplest $SU(2)$ representation, which is compatible with the Cosmological…

宇宙学与河外天体物理 · 物理学 2025-05-20 Marco Frasca , Anish Ghoshal , Massimilano Rinaldi

We first consider the Einstein-aether theory with a gravitational coupling and a Lagrange multiplier field, and then consider the non-minimally coupled quintessence field theory with Lagrange multiplier field. We study the influence of the…

宇宙学与河外天体物理 · 物理学 2015-05-18 Changjun Gao , Yan Gong , Xin Wang , Xuelei Chen

We propose a dynamical (quintessence) model of dark energy in the current universe with a renormalizable (Higgs-like) scalar potential. We prove the viability of our model (after fine tuning) for the certain range of the average scalar…

高能物理 - 理论 · 物理学 2015-03-17 Sergei V. Ketov , N. Watanabe

Generalised axion-like scalar fields provide a well-motivated framework for describing the late-time acceleration of the Universe. As the field evolves, it rolls down its potential and, depending on its mass and initial conditions, it may…

宇宙学与河外天体物理 · 物理学 2026-03-30 Mariam Bouhmadi-López , Carlos G. Boiza

Physics invites the idea that space contains energy whose gravitational effect approximates that of Einstein's cosmological constant, Lambda; nowadays the concept is termed dark energy or quintessence. Physics also suggests the dark energy…

天体物理学 · 物理学 2008-11-26 P. J. E. Peebles , Bharat Ratra

In a recent paper we showed that a quintessence scalar field plus a dissipative matter fluid can drive late cosmic accelerated expansion and simultaneously solve the coincidence problem [1]. In this brief report we extend this result to the…

天体物理学 · 物理学 2009-11-07 Luis P. Chimento , Alejandro S. Jakubi , Diego Pavon

Can local fluctuations of a ``Quintessence'' scalar field play a dynamical role in the gravitational clustering and cosmic structure formation process? We address this question in the general framework of scalar-tensor theories of gravity.…

天体物理学 · 物理学 2009-11-10 F. Perrotta , S. Matarrese , M. Pietroni , C. Schimd

Recently, attempts have been made to understand the apparent near coincidence of the present dark energy and matter energy in terms of a dynamical attractor-like solution for the evolution of a scalar field. In these models the field…

天体物理学 · 物理学 2009-11-06 M. Yahiro , G. J. Mathews , K. Ichiki , T. Kajino , M. Orito

We study static configurations of dark matter coupled to a scalar field responsible for the dark energy of the Universe. The dark matter is modelled as a Fermi gas within the Thomas-Fermi approximation. The mass of the dark matter particles…

天体物理学 · 物理学 2009-11-13 N. Brouzakis , N. Tetradis

In this work it is investigated the evolution of a Universe where a scalar field, non-minimally coupled to space-time curvature, plays the role of quintessence and drives the Universe to a present accelerated expansion. A non-relativistic…

广义相对论与量子宇宙学 · 物理学 2009-11-11 J. B. Binder , G. M. Kremer