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Related papers: Quintessence as k-essence

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Models where the accelerated expansion of our Universe is caused by a quintessence scalar field are reviewed. In the framework of high energy physics, the physical nature of this field is discussed and its interaction with ordinary matter…

Astrophysics · Physics 2009-06-23 Jerome Martin

At present we know nothing about the nature of the dark energy accounting for about 70% of the energy density of the Universe. One possibility is that the dark energy is provided by an extremely light field, the quintessence, rolling down…

High Energy Physics - Phenomenology · Physics 2009-11-07 D. J. H. Chung , L. L. Everett , A. Riotto

Recent observations suggest that the accelerated expansion of the Universe at late times is caused by a temporally changing dark energy component, rather than the constant one in the standard $\Lambda$CDM scenario. In this context…

General Relativity and Quantum Cosmology · Physics 2025-11-05 Artur Alho , Elsa Bernholm , Claes Uggla

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…

High Energy Physics - Theory · Physics 2015-03-17 Sergei V. Ketov , N. Watanabe

Various astronomical observations point towards the evidence for dark energy. One of the most mysterious problem is the coincidence problem: why dark energy becomes dominant only recently. We present a scenario based on extended…

Astrophysics · Physics 2009-11-06 Takeshi Chiba

Dark energy models with non-canonical kinetic energy terms, k-essence, can have dynamical and sound speed properties distinct from canonical scalar fields, quintessence. Concentrating on purely kinetic term Lagrangians, which can be…

Astrophysics · Physics 2008-11-26 Roland de Putter , Eric V. Linder

The archetypal theory of dark energy is quintessence: a minimally coupled scalar field with a canonical kinetic energy and potential. By studying random potentials we show that quintessence imposes a restricted set of priors on the equation…

Cosmology and Nongalactic Astrophysics · Physics 2014-12-11 David J. E. Marsh , Philip Bull , Pedro G. Ferreira , Andrew Pontzen

We consider a model of dark energy/matter unification based on a k-essence type of theory similar to tachyon condensate models. Using an extension of the general relativistic spherical model which incorporates the effects of both pressure…

General Relativity and Quantum Cosmology · Physics 2017-08-23 Neven Bilic , Gary B. Tupper , Raoul D. Viollier

We consider multiple k-essence sources and obtain the conditions their kinetic functions must satisfy so that purely kinetic k-essences lead to models with phantom barrier crossing. After that, we show that polynomial kinetic functions…

Astrophysics · Physics 2009-11-11 Luis P. Chimento , Ruth Lazkoz

We explore quintessence models of dark energy which exhibit non-minimal coupling between the dark matter and the dark energy components of the cosmic fluid. The kind of coupling chosen is inspired in scalar-tensor theories of gravity. We…

Astrophysics · Physics 2009-11-13 Tame Gonzalez , Genly Leon , Israel Quiros

There are a number of mathematical theorems in the literature on the dynamics of cosmological models with accelerated expansion driven by a positive cosmological constant $\Lambda$ or a nonlinear scalar field with potential $V$…

General Relativity and Quantum Cosmology · Physics 2009-11-11 Alan D. Rendall

We consider a connection between the holographic dark energy density and the kinetic k-essence energy density in a flat FRW universe. With the choice $c\geq1$, the holographic dark energy can be described by a kinetic k-essence scalar field…

General Relativity and Quantum Cosmology · Physics 2009-09-28 Norman Cruz , Pedro F. Gonzalez-Diaz , Alberto Rozas-Fernandez , Guillermo Sanchez

In this work we present a model of the universe in which dark energy is modelled explicitely with both a dynamical quintessence field and a cosmological constant. Our results confirm the possibility of a future collapsing universe (for a…

Astrophysics · Physics 2009-11-07 Rolando Cardenas , Tame Gonzalez , Yoelsy Leiva , Osmel Martin , Israel Quiros

We analyze the coupled quintessence in the light of the linear dynamical systems theory, with two different interactions: i) proportional to the energy density of the dark energy and ii) proportional to the sum of the energy densities of…

General Relativity and Quantum Cosmology · Physics 2017-05-09 Fabrizio F. Bernardi , Ricardo G. Landim

We construct the non-canonical kinetic term of a k-essence field directly from the effective equation of state function $w_k(z)$, which describes the properties of the dark energy. Adopting the usual parametrizations of equation of state we…

Astrophysics · Physics 2011-04-12 Hui Li , Zong-Kuan Guo , Yuan-Zhong Zhang

We explicitly construct the k-essence models which reproduce the arbitrary FRW cosmology, that is, the arbitrary time-development of the scale factor or the Hubble rate. The k-essence model includes scalar quintessence model, tachyon dark…

High Energy Physics - Theory · Physics 2010-04-30 Jiro Matsumoto , Shin'ichi Nojiri

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.…

General Relativity and Quantum Cosmology · Physics 2015-06-15 Shinji Tsujikawa

K-essence has been proposed as a possible means of explaining the coincidence problem of the Universe beginning to accelerate only at the present epoch. We carry out a comprehensive dynamical systems analysis of the k-essence models given…

Astrophysics · Physics 2009-11-07 Michael Malquarti , Edmund J Copeland , Andrew R Liddle

Recent observations suggest that a large fraction of the energy density of the universe has negative pressure. One explanation is vacuum energy density; another is quintessence in the form of a scalar field slowly evolving down a potential.…

Astrophysics · Physics 2009-09-15 Ivaylo Zlatev , Limin Wang , Paul J. Steinhardt

Dark energy, the main constituent in our expanding universe, responsible for its acceleration, is currently being observed with unprecedented precision through various experiments. While several cosmological models can fit this latest data,…

High Energy Physics - Theory · Physics 2026-04-10 David Andriot